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University of Wollongong Research Online University of Wollongong esis Collection University of Wollongong esis Collections 2013 e electronic and optical properties of graphene Shareef Faik Sultan Al-Tikrity University of Wollongong Research Online is the open access institutional repository for the University of Wollongong. For further information contact the UOW Library: [email protected] Recommended Citation Al-Tikrity, Shareef Faik Sultan, e electronic and optical properties of graphene, Doctor of Philosophy thesis, School of Engineering Physics, University of Wollongong, 2013. hp://ro.uow.edu.au/theses/4013
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Page 1: University of Wollongong Thesis Collection University of … · 2018-12-12 · University have been indispensable. I also thank the faculty of engineering and school of physics for

University of WollongongResearch Online

University of Wollongong Thesis Collection University of Wollongong Thesis Collections

2013

The electronic and optical properties of grapheneShareef Faik Sultan Al-TikrityUniversity of Wollongong

Research Online is the open access institutional repository for theUniversity of Wollongong. For further information contact the UOWLibrary: [email protected]

Recommended CitationAl-Tikrity, Shareef Faik Sultan, The electronic and optical properties of graphene, Doctor of Philosophy thesis, School of EngineeringPhysics, University of Wollongong, 2013. http://ro.uow.edu.au/theses/4013

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School of Engineering Physics

Title of the Thesis

The Electronic and Optical Properties

of Graphene

Students Full Name

Shareef Faik Sultan Al-Tikrity

"This thesis is presented as part of the requirements for the

award of the Degree of

Doctor of Philosophy of the

University of Wollongong"

Thesis supervisor: A/Professor Rodney Vickers

Professor Chao Zhang

June/201

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Certification

I, Shareef Faik Sultan Al-Tikrity, declare that this thesis, submitted in

partial fulfilment of the requirements for the award of Doctor of

Philosophy, in the School of Engineering Physics, University of

Wollongong, is wholly my own work unless otherwise referenced or

acknowledged. The document has not been submitted for qualifications at

any other academic institution.

Shareef Faik Sultan Al-Tikrity

30 July 2013

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In The Name Of Allah The Beneficent The Merciful

It is Allah who created the heavens and the earth and whatever is between them in six days; then He established Himself above the Throne. You have not besides Him any protector or any intercessor; so will you not be reminded?

He arranges [each] matter from the heaven to the earth; then it will ascend to Him in a Day, the extent of which is a thousand years of those which you count. Surat As-Sajdah (The Prostration) – سورة السجدة

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DEDICATED TO

To the utmost knowledge lighthouse, to our greatest and most

honoured prophet Mohamed – (May peace and grace from Allah

be upon him).

To whom he strives to bless comfort and welfare and never stints

what he owns to push me in the success way who taught me to

promote life stairs wisely and patiently, to my dearest father

To the spring that never stops giving, to my mother who weaves

my happiness with strings from her merciful heart... to my

mother.

To my Brothers and Sisters

To my Lovely Wife

To my Nephew and Niece

To my Daughter (Deema) and my Son (Abd Al-mumin)

To my Relatives

To my friends

I guide this work

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ABSTRACT

This thesis describes theoretical and experimental studies into the optical response

of single and multiple layer graphene in the terahertz to infrared regime and provides a

description of some the unique characteristics of graphene.

In this work, the Schrödinger time-dependent equation is employed for gapless

and gapped graphene in monolayers and bilayers to specify the optical and electronic

characteristics and describe the electronic transitions in the structuring of the

honeycomb lattice that depend on the Hamiltonian equation and include applied

electric field. The energy band dispersion and wave function are calculated by using a

quantum mechanical approach, together with the tight-binding model, and a

comparison with Bloch's theory is included in order to satisfy the theoretical details

and provide a description of the low energy bands of graphene. Furthermore, this

procedure has been used to study the interband transitions. The Boltzmann formula

has also been used to describe the intraband transitions. To analyze our results, models

for the optical response of graphene single layers and bilayer are taken into account,

based on the electronic system described by the Fermi-Dirac distribution at different

temperatures and in the most important frequency regime.

The linear and nonlinear optical conductivity and current density have been

calculated to first and the third order for single-layer gapped and gapless graphene and

bilayer graphene. It is demonstrated that the third order nonlinear response includes

single frequency and frequency tripling nonlinear terms.

In the present results, single layer graphene on a substrate layer shows a

strong response in the p-n junction regime in the nonlinear optical conductivity. It is

also shown that the conductivity can be negative within a limited range of frequencies,

depending on the bias voltage ( and when . In the terahertz regime, the

negative conductivity increases with increasing relaxation time and gate voltage, and

with decreasing temperature. In this kind of p-n junction, the nonlinear optical

response in the gapped and gapless graphene shows a strong response under forward

bias. Also, the negative conductance provides a unique mechanism for photon

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generation in graphene and could be used for developing coherent terahertz radiation

sources.

In the both the weak field and the strong field Fermi-Dirac distribution, the linear

and nonlinear current density of single-layer gapped and gapless graphene has been

calculated as a function of temperature. In gapless graphene, the nonlinear current

effect increases with temperature up to room temperature, and is very much stronger

than the linear current density. The third order nonlinear optical response in strong

field is asymmetric between and and can be stronger than that in weak

field. The nonlinear optical response in gapped graphene is stronger than in gapless

graphene under weak field at zero to finite temperature, and it increases with

increasing temperature with a finite gap. The linear and the nonlinear optical responses

in gapped graphene are affected by the strong field (under the Fermi-Dirac

distribution) but the opposite is true with the linear gapless graphene.

For bilayer graphene, the optical conductivity can be affected by changing the

temperature. Increasing the temperature from low to room temperature leads to a

decrease in the optical conductivity where there is an electric field of 1000 V/cm. In

addition, the nonlinear optical response decreases gradually with increasing frequency.

Also, the single frequency nonlinear response is greater than the frequency tripled

nonlinear response in different frequency ranges.

The critical electric field plays an important role in equalizing the linear and

nonlinear optical responses at a specific field of ~ . Also, the critical field

increases with increasing frequency or temperature.

It is demonstrated that the second order response in single and bilayer gapless and

gapped graphene is equal to zero in both the strong field and the weak field regimes

due to the inversion symmetry of the graphene structure.

Transmittance spectra from the terahertz to the infrared range in the multilayer

sample (Graphene on substrate) and single layer samples (graphene only) at room

temperature could be feasibly collected and were useful due to the high mobility of

electrons in graphene at room temperature. Fourier transform spectroscopy is used to

describe the transmittance of graphene and graphite films under room pressure and in

vacuum. In the present results, graphene multilayer on Si substrate has low resistance

at room temperature, less than that of the silicon alone. In addition, a new method was

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developed to calculate the transmittance and reflectance through multiple layers. This

method is demonstrated to be more accurate than the classic (general) method. The

theoretical and experimental results also show good convergence at short and long

wavelengths.

Finally, the highly tunable and strong optical properties of graphene-based

materials make graphene a new alternative candidate to most of the semiconductor

materials. Also, the high transmittance and low resistance of graphene represent a

remarkable result. Therefore, we suggest that graphene could be a candidate for

developing optoelectronics devices and graphene-based optical applications, as well as

being useful for building innovative devices for nonlinear terahertz applications.

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ACKNOWLEDGEMENTS

In the name of Allah, the most Merciful, the most Gracious. I am thankful to

Allah, who supplied me with the courage, the guidance, and the love to complete this

thesis. Also, I cannot forget the ideal man, peace man of the world and most

respectable personality, Prophet Mohammed (Peace Be Upon Him).

First and foremost I offer my sincerest gratitude to my supervisors, Professor

Chao Zhang and A/Professor Rodney Vickers, whose have supported me throughout

my thesis with their patience, knowledge, excellent guidance, caring and providing me

with an excellent atmosphere for doing this thesis.

I would like to offer my gratitude to the Ministry of Higher Education and

Scientific Research of the Republic of Iraq for the Scholarship awarded and the

financial supports. For that reason, I would like to express my sincere thanks and

gratitude to my country.

I would like to acknowledge the academic and technical support of the University

of Wollongong and its staff. The library facilities and computer facilities of the

University have been indispensable. I also thank the faculty of engineering and school

of physics for their support and assistance since the start of my PhD. work in 2009,

especially the dean, sub-dean, head of school and head of postgraduate studies.

I would like to thank Yee Sin Ang, Anthony Wright and Steven for their kindness,

friendship and support, together with the other friends of school of physics. Many

thanks Prof. Roger Lewis and other workers in the laboratory of physics for helping

me.

I wish to express my sincere thanks and gratitude to the editor language Tania

Silver, who helped me to linguistic correction and proofreading in my thesis. Many

thank Dr. Alisa Percy in the Learning Development for helping me to proofreading in

my research.

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Most importantly, I would especially like express my sincere thanks and gratitude

to my parent for their love, support and encouragement throughout my studies. I

would also like to thank my sisters, brothers, my wife's family and my relatives. They

were always supporting me and encouraging me with their best wishes. I especially

must restate my sincere appreciation to my dear wife for her love, encouragement and

support during my studies. She was always stood by me through the good times and

bad. I would also like to thank my beloved daughter and son, whose gave me

happiness, hope and ambition.

Last, but by no means least, I thank my friends in Iraq, Australia and elsewhere

for their support and encouragement throughout. For any errors or inadequacies that

may remain in this work, of course, the responsibility is entirely my own. Finally, I

wish to offer special thanks to all those who have given me assistance and support

during this Work. I would never have been able to finish my thesis without their

guidance, support and help.

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TABLE OF CONTENTS

Certification ................................................................................................................... i

In The Name Of Allah The Beneficent The Merciful .................................................. ii

Dedicated to ................................................................................................................ iii

ABSTRACT ................................................................................................................ iv

ACKNOWLEDGEMENTS ....................................................................................... vii

TABLE OF CONTENTS ............................................................................................ ix

LIST OF FIGURES .................................................................................................... xii

1 Introduction to the Electronic and Optical Properties of Graphene......................... 1

1.1 Introduction .................................................................................................... 1

1.2 Graphene: literature review and background ................................................. 2

1.3 Carbon atom and structure of graphene from the chemical viewpoint .......... 5

1.4 Geometry of the band structure of graphene's honeycomb lattice from the

physical viewpoint .................................................................................................. 10

1.4.1 Bloch wave function and tight binding approach ........................................... 12

1.4.2 Single layer graphene ..................................................................................... 17

1.4.3 Bilayer graphene ............................................................................................. 26

1.5 Scope of thesis ............................................................................................. 29

2 Nonlinear Optical Conductance of a Single layer Graphene p-n Junction in the

Terahertz Regime ................................................................................................... 31

2.1 Introduction .................................................................................................. 31

2.2 Single layer gapless graphene p-n junction ................................................. 32

2.1.1 Intraband Transitions ...................................................................................... 34

2.1.2 Inter band transitions ...................................................................................... 36

2.1.2.1 Linear conductivity ......................................................................................... 40

2.1.2.2 Nonlinear conductivity ................................................................................... 44

2.3 Single-layer gapped graphene p-n junction ................................................. 51

2.3.1 Intraband Transitions ...................................................................................... 52

2.3.2 Interband Transitions ...................................................................................... 53

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2.3.3 Linear conductivity ......................................................................................... 56

2.3.4 Nonlinear conductivity ................................................................................... 59

2.4 Conclusion ................................................................................................... 63

3 Strong Terahertz Photon Mixing in Graphene ....................................................... 65

3.1 Introduction .................................................................................................. 65

3.2 Photon mixing in single layer gapless graphene .......................................... 67

3.2.1 Formalism and theory ..................................................................................... 68

3.2.2 Linear optical response of gapless graphene .................................................. 71

3.2.3 Nonlinear optical response of gapless graphene ............................................. 72

3.2.4 Critical electric field and Photon mixing effect .............................................. 75

3.2.5 Strong optical response photon-mixing in gapless graphene under the strong

field of hot Dirac Fermions ............................................................................................ 78

3.3 Photon mixing in single-layer gapped graphene.......................................... 84

3.3.1 Formalism and theory ..................................................................................... 85

3.3.2 Linear optical response of gapped graphene .................................................. 87

3.3.3 Nonlinear optical response of gapped graphene ............................................. 88

3.3.4 Critical electric field and Photo mixing effect ................................................ 90

3.3.5 Strong optical response photon-mixing in gapped graphene under the strong

field of hot Dirac Fermions ............................................................................................ 92

3.4 Conclusion ................................................................................................... 94

4 Nonlinear Optical Properties of Bilayer Graphene in the Terahertz Regime ........ 96

1.4 Introduction .................................................................................................. 96

1.4 Formalism and theory of Hamiltonian in bilayer graphene under the low-

energy ..................................................................................................................... 99

4.3 Current density formalism and theory ....................................................... 104

4.3.1 Velocity operator formalism in the current density equation ....................... 105

4.4 Linear optical response of bilayer gapless graphene ................................. 106

4.5 Non-linear optical response of bilayer gapless graphene .......................... 109

4.6 Results and discussion ............................................................................... 112

4.7 Conclusion ................................................................................................. 117

5 EXPERIMENTAL TECHNIQUES ..................................................................... 119

5.1 Introduction ................................................................................................ 119

5.2 Bomem Hardware ...................................................................................... 119

5.2.1 KBr Beam Splitters ..................................................................................... 124

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5.2.2 Broad Band Beam Splitters .......................................................................... 124

5.3 Bomem software ........................................................................................ 126

5.3.1 Interferogram analysis and Fourier transforms ............................................. 128

5.3.2 Definition of Fourier transforms theory from a mathematical viewpoint..... 130

5.4 Optical Cryostats........................................................................................ 132

5.5 Detectors .................................................................................................... 134

5.5.1 Bolometer Detector ....................................................................................... 134

5.5.2 MCT Detector ............................................................................................... 136

5.6 Sample preparation .................................................................................... 137

6 Experiment ........................................................................................................... 139

6.1 Introduction ................................................................................................ 139

6.2 Electric measurements ............................................................................... 142

6.3 Theoretical model of transmittance and reflection .................................. 148

6.4 Transmittance of single layer thin metal film ........................................... 154

6.5 Transmittance through a single layer of thin metal deposited on a substrate

156

6.6 Measuring the transmittance of silicone with and without graphene. ....... 161

6.7 Measuring the transmittance of Pure Graphene ......................................... 165

6.8 Results and Discussion .............................................................................. 168

6.9 Conclusion ................................................................................................. 173

7 Conclusion ........................................................................................................... 175

REFERENCES ......................................................................................................... 180

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LIST OF FIGURES

FIGURE ‎1.1 (A) SCHEMATIC REPRESENTATION OF AND BONDS IN GRAPHENE [28];

(B) SCHEMATIC VIEW OF HYBRIDISATION OF CARBON ATOM; (C)

GRAPHENE IS A CARBON ALLOTROPE WITH A TWO-DIMENSIONAL HONEYCOMB

LATTICE STRUCTURE; (D) TYPICAL HEXAGON FROM THE GRAPHENE LATTICE

SURROUNDED BY SIX CARBON ATOMS WITH ONE CARBON ATOM IN EACH

CORNER. ................................................................................................................ 6

FIGURE ‎1.2. (A) LATTICE STRUCTURE OF GRAPHITE AS GRAPHENE MULTILAYER. (B)

FULLERENES (C60) ARE MOLECULES CONSISTING OF WRAPPED GRAPHENE. (C)

CARBON NANOTUBE AS A ROLLED UP GRAPHENE LAYER. (D) UNIT CELL OF THE

DIAMOND CUBIC CRYSTAL STRUCTURE. ................................................................. 9

FIGURE ‎1.3. (A): GRAPHENE HONEYCOMB LATTICE STRUCTURE WITH THE TWO

GRAPHENE SUBLATTICES, AND PRIMITIVE UNIT VECTORS AND OTHER UNIT

CELLS AS DEFINED ABOVE. (B) HEXAGONAL STRUCTURE OF GRAPHENE WITH

RECIPROCAL LATTICE VECTOR AND THE FIRST BRILLOUIN ZONE. ........................ 11

FIGURE ‎1.4. ENERGY DISPERSION IN THE HONEYCOMB GRAPHENE LATTICE. (A)

LEFT, THE ENERGY BANDS OF A GRAPHENE MONOLAYER SHEET IN 3D. RIGHT,

THE ENERGY DISPERSION OF GRAPHENE AT THE K-POINT, WHICH IS KNOWN AS

THE DIRAC CONE. (B) COMPARISON OF AB-INITIO MODEL AND TIGHT BANDING

MODEL OF GRAPHENE, SHOWING GOOD AGREEMENT AT LOW ENERGIES [54]. ...... 16

FIGURE ‎1.5. OPTICAL MICROSCOPE IMAGE OF A GRAPHENE FLAKE: (A) THREE

REGIONS CAN BE IDENTIFIED: I, SINGLE-LAYER GRAPHENE; II, MULTILAYER

GRAPHENE; AND III, THE SILICON-DIOXIDE-COATED SUBSTRATE. (B) IMAGE OF

THE SAME FLAKE AFTER THE DEPOSITION OF AN 18-NM LAYER OF GOLD. (C)

STM IMAGE OF A SINGLE-LAYER GRAPHENE FILM ON THE SILICON DIOXIDE

SURFACE. (D) THE FULL HEXAGONAL SYMMETRY EXPECTED OF AN ISOLATED

SINGLE LAYER GRAPHENE SHEET. (E) IMAGE OF THE MULTILAYER PORTION OF

THE SAMPLE [68]. ................................................................................................ 22

FIGURE ‎1.6. THE FINITE-WIDTH HONEYCOMB STRUCTURE OF GRAPHENE

NANORIBBONS: (A) ZIGZAG EDGE OF GRAPHENE NANORIBBONS; (B) ARMCHAIR

EDGE OF GRAPHENE NANORIBBONS. .................................................................... 24

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FIGURE ‎1.7. (A) SCHEMATIC DIAGRAM OF LATTICE STRUCTURE OF BILAYER

GRAPHENE IN (A) A PLANE AND (B) A SIDE VIEW OF THE CRYSTAL STRUCTURE

[86]. (C) SCHEMATIC OF LOW ENERGY BANDS AROUND K POINTS. ...................... 27

FIGURE ‎2.1. SCHEMATIC DIAGRAM OF THE BAND STRUCTURE OF GRAPHENE P-N

JUNCTION. (A) ILLUSTRATES THE DUAL GATE VOLTAGE OF GRAPHENE IN THE P-

N JUNCTION REGIME [92]. (B) ENERGY BAND DIAGRAM OF SINGLE LAYER

GAPLESS GRAPHENE WITH BIAS VOLTAGE IN BOTH SIDES ( P REGION AND N

REGION). .............................................................................................................. 32

FIGURE ‎2.2. THE TOTAL REAL PART OF THE LINEAR OPTICAL CONDUCTANCE OF A

SINGLE-LAYER GAPLESS GRAPHENE P-N JUNCTION OSCILLATING WITH

FREQUENCY IN UNIT OF WITH DIFFERENT VALUES OF THE

RELAXATION TIME WHEN AND AT T = 77K. ........... 43

FIGURE ‎2.3. THE REAL PART OF THE TOTAL OPTICAL CONDUCTIVITY OF THE

GRAPHENE P-N JUNCTION AS A FUNCTION OF FREQUENCY FOR DIFFERENT

ELECTRIC FIELD INTENSITY, WITH Τ = 10 PS, MEV, AND BIAS VOLTAGE

. ....................................................................................................... 50

FIGURE ‎2.4. THE RATIO OF THE REAL PART OF THE NONLINEAR AND LINEAR OPTICAL

CONDUCTIVITY VS. THE ELECTRIC FIELD INTENSITY, WITH , BIAS

VOLTAGE AND THE . ........................................................ 50

FIGURE ‎2.5. SCHEMATIC DIAGRAM OF THE BAND STRUCTURE OF GAPPED SINGLE-

LAYER GRAPHENE IN THE P-N JUNCTION REGIME UNDER MODERATE ELECTRIC

FIELD. .................................................................................................................. 52

FIGURE ‎2.6. THE REAL PART OF LINEAR OPTICAL CONDUCTIVITY DEPENDENCE ON

THE FREQUENCY WITH DIFFERENT BAND GAP , WHERE ,

AND THE BIAS VOLTAGE AT T=77 K. ................................. 58

FIGURE ‎2.7. NORMALIZED REAL PART OF THE LINEAR CONDUCTIVITY VS. THE

FREQUENCY CALCULATED FOR DIFFERENT TEMPERATURES BELOW

WITH , AND THE BIAS VOLTAGE

. ................................................................................................................. 58

FIGURE ‎2.8. THE REAL PART OF THE TOTAL LINEAR AND NONLINEAR OPTICAL

CONDUCTIVITY OF THE GAPPED GRAPHENE P-N JUNCTION AS A FUNCTION OF

FREQUENCY. ........................................................................................................ 61

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FIGURE ‎2.9. THE RATIO OF THE REAL PART OF THE NONLINEAR TO THE LINEAR

OPTICAL CONDUCTIVITY IN GAPPED GRAPHENE AGAINST THE ELECTRIC fiELD

INTENSITY, WITH , BIAS VOLTAGE , AND

THE BAND GAP . ................................................................................ 62

FIGURE ‎3.1. SCHEMATIC DIAGRAM OF THE BAND STRUCTURE OF SINGLE LAYER

GAPLESS GRAPHENE AND THE NONLINEAR PHOTON MIXING PROCESS WHEN

SIGN OF THE ENERGY STATE . .................................................................. 67

FIGURE ‎3.2. TEMPERATURE DEPENDENCE OF THE NORMALIZED THIRD-ORDER

NONLINEAR CURRENT DENSITY FOR AT ................................... 74

FIGURE ‎3.3. TEMPERATURE DEPENDENCE OF THE NORMALIZED THIRD-ORDER

NONLINEAR CURRENT DENSITY FOR AT ................................... 74

FIGURE ‎3.4. AND THE CRITICAL FIELD EC (INSET) AS FUNCTIONS OF TEMPERATURE

IN GAPLESS GRAPHENE FOR DIFFERENT WHEN ............................. 77

FIGURE ‎3.5. TEMPERATURE DEPENDENCE OF THE CRITICAL ELECTRIC FIELD AT

AND FOR DIFFERENT CRITICAL FIELD CASES: (I) WEAK

FIELD (II) STRONG CRITICAL FIELD BOTH UNDER SDF. THE INSET

SHOWS THE TEMPERATURE DEPENDENCE OF IN THE STRONG FIELD OF HOT

DIRAC FERMIONS. ................................................................................................ 83

FIGURE ‎3.6. TEMPERATURE DEPENDENCE OF THE THIRD ORDER NONLINEAR

CURRENT DENSITY AT FINITE TEMPERATURE ( NORMALISED BY THAT AT

IN THE SDF REGIME WITH THREE DIFFERENT CHEMICAL POTENTIALS. ...... 83

FIGURE ‎3.7. BAND-GAP DEPENDENCE OF WITH THREE DIFFERENT AT ZERO

TEMPERATURE AND . .......................................................................... 91

FIGURE ‎4.1. (A) SCHEMATIC DIAGRAM OF THE ATOMIC STRUCTURE OF BILAYER

GRAPHENE. SOLID LINES INDICATE THE TOP LAYER, AND DASHED LINES

INDICATE THE BOTTOM LAYER. (B) SCHEMATIC DIAGRAM OF THE ATOMIC

STRUCTURE IN BILAYER GRAPHENE WITH THREE HOPPING PARAMETERS. IS

THE HOPPING PARAMETER BETWEEN NEAREST-NEIGHBOUR SITES WITHIN EACH

LAYER. REPRESENTS THE HOPPING BETWEEN A1 AND B2, AND BETWEEN

B1 AND A2. ......................................................................................................... 98

FIGURE ‎4.2. SCHEMATIC DIAGRAM OF THE FOUR LOW ENERGY BANDS AROUND K

POINTS. .............................................................................................................. 102

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FIGURE ‎4.3. LINEAR OPTICAL CONDUCTANCE AS A FUNCTION OF FREQUENCY AT

ZERO TEMPERATURE. ......................................................................................... 114

FIGURE ‎4.4. NONLINEAR OPTICAL CONDUCTANCE AS A FUNCTION OF FREQUENCY AT

ZERO AND ROOM TEMPERATURE, WITH THE ELECTRIC FIELD SET AT 1000 V/CM.114

FIGURE ‎4.5. NORMALIZED NONLINEAR CONDUCTIVITY IN UNITS OF VERSUS

TEMPERATURE AT FIELD OF 600 V/CM AND 1 THZ FREQUENCY. ........................ 115

FIGURE ‎4.6. CRITICAL ELECTRIC FIELDS AT ZERO AND ROOM TEMPERATURE AS A

FUNCTION OF THE FREQUENCY WITHIN THE RANGE OF 0-5 THZ. ....................... 115

FIGURE ‎4.7. CRITICAL FIELD VS. TEMPERATURE AT FREQUENCY OF 1 THZ. ............. 116

FIGURE ‎5.1. THE BOMEM DA8 FTIR INTERFEROMETER SPECTROMETER. ................. 122

FIGURE ‎5.2. (A) MIDDLE SECTION OF THE BOMEM DA8 FTIR SPECTROMETER

CONTAINING THE BEAM SWITCHING COMPARTMENT, THE SAMPLE

COMPARTMENT, AND THE TWO DETECTOR MODULES. (B) OPTICAL

CONFIGURATION OF THE BOMEM DA8 FTIR SPECTROMETER [144,145,147]. .. 123

FIGURE ‎5.3. BEAM-SPLITTER RANGE IN WAVENUMBERS (CM-1). ............................... 125

FIGURE ‎5.4. THE PCDA COLLECT WINDOW SHOWING THE CURRENT STATUS AND

OPERATION CONDITION OF THE SPECTROMETER. ................................................ 127

FIGURE ‎5.5. (A) MICHELSON INTERFEROMETER. THE RESULTS CAN BE (B) A

SYMMETRICAL INTERFEROGRAM AND (C) AN ASYMMETRICAL INTERFEROGRAM.129

FIGURE ‎5.6. OPTISTAT − AN OPTICAL CONTINUOUS FLOW CRYOSTAT [15]. ............... 133

FIGURE ‎5.7. THE BOLOMETER DETECTOR. ................................................................. 135

FIGURE ‎5.8. SPECTRA OF THREE TYPES OF FILTERS IN THE BOLOMETER DETECTOR

[148,160,161]. .................................................................................................. 135

FIGURE ‎5.9. MCT DETECTOR [148,162, 163]. ........................................................... 136

FIGURE ‎5.10. (A) GRAPHENE LIQUID; (B) SOLID GRAPHENE. ...................................... 138

FIGURE ‎5.11. (A) DIMENSIONS OF SILICON A661 NTD; (B) SILICON A661 NTD

COATED BY GRAPHENE. ..................................................................................... 138

FIGURE ‎6.1. SCHEMATIC DIAGRAM OF THE ELECTROMAGNETIC SPECTRUM. .............. 141

FIGURE ‎6.2. SCHEMATIC DIAGRAM SHOWING THE MECHANISMS OF REFLECTION,

ABSORPTION, AND TRANSMISSION THROUGH THE SAMPLE TO PRODUCE THE

OUTPUT SPECTRUM. ........................................................................................... 141

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FIGURE ‎6.3. SCHEMATIC DIAGRAM OF THE SIMPLE OPTICAL AND ELECTRICAL

SYSTEM TO MEASURE THE ELECTRICAL RESISTANCE OF THE SAMPLE................. 143

FIGURE ‎6.4. CURRENT-VOLTAGE CURVES OF SI A661 WITH AND WITHOUT

GRAPHENE AT ROOM TEMPERATURE. ................................................................. 144

FIGURE ‎6.5. CURRENT-VOLTAGE CURVES AT ROOM TEMPERATURE FOR THE SI

SUBSTRATE WITH AND WITHOUT GRAPHENE FILM, WITH BLACK POLYTHENE

FILTER IN THE PATH OF THE INFRARED BEAM. .................................................... 144

FIGURE ‎6.6. VOLTAGE DEPENDENCE OF THE CURRENT THROUGH SI A661 WITH AND

WITHOUT GRAPHENE AT NITROGEN TEMPERATURE. ........................................... 145

FIGURE ‎6.7. TEMPERATURE DEPENDENCE OF THE VOLTAGE UNDER INFRARED

RADIATION FOR GRAPHENE FOR DIFFERENT VALUES OF CURRENT. .................... 146

FIGURE ‎6.8. TEMPERATURE DEPENDENCE OF THE VOLTAGE OF GRAPHENE WITH AND

WITHOUT INFRARED RADIATION FOR 1 MA CURRENT......................................... 147

FIGURE ‎6.9. CURRENT DEPENDENCE OF THE VOLTAGE OF GRAPHENE AT DIFFERENT

TEMPERATURES UNDER INFRARED RADIATION. .................................................. 147

FIGURE ‎6.10. THE ELECTRIC FIELD OF THE LIGHT IS PERPENDICULAR TO THE PLANE

OF INCIDENCE AND THE MAGNETIC FIELD IS PARALLEL TO IT. ............................ 148

FIGURE ‎6.11. THE ELECTRIC FIELD IS PARALLEL TO THE PLANE OF INCIDENCE, AND

THE MAGNETIC FIELD IS PERPENDICULAR TO IT. ................................................. 150

FIGURE ‎6.12. TRANSMISSION, REFLECTION, AND ABSORPTION FOR A SINGLE-LAYER

THIN FILM WITHOUT A SUBSTRATE. .................................................................... 155

FIGURE ‎6.13. TRANSMITTANCE, REFLECTION, AND ABSORPTION FOR A THIN FILM ON

A THICK, TRANSPARENT SUBSTRATE. THE REFLECTANCE IN THE SUBSTRATE IS

NOT INCLUDED. .................................................................................................. 157

FIGURE ‎6.14. TRANSMITTANCE, REFLECTANCE, AND ABSORPTION OF THIN FILM ON A

THICK, TRANSPARENT SUBSTRATE. THE REFLECTANCE IN THE SUBSTRATE IS

INCLUDED. ......................................................................................................... 158

FIGURE ‎6.15. RAW SPECTRA OF THE TRANSMITTED RADIATION THROUGH SI

SAMPLES WITH AND WITHOUT GRAPHENE. ......................................................... 162

FIGURE ‎6.16. SPECTRA OF THE TRANSMITTED RADIATION THROUGH SI SAMPLES

WITH AND WITHOUT GRAPHENE, AND THE REFERENCE SPECTRUM WITH NO

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SAMPLE IN THE BEAM PATH (INSET), USING FOURIER TRANSFORMS WITH

BOLOMETER AND BROADBAND BEAM SPLITTER. ................................................ 163

FIGURE ‎6.17. SPECTRA OF THE TRANSMITTED RADIATION THROUGH SI SAMPLES

WITH AND WITHOUT GRAPHENE, AND THE REFERENCE SPECTRUM WITH NO

SAMPLE IN THE BEAM PATH, USING FOURIER TRANSFORMS WITH MCT

DETECTOR AND KBR BEAM SPLITTER. ............................................................... 163

FIGURE ‎6.18. RATIO OF THE TRANSMITTED RADIATION THROUGH SI WITH AND

WITHOUT GRAPHENE TO THE REFERENCE SPECTRUM WITH NO SAMPLE IN THE

BEAM PATH, WITH BOLOMETER AND BROADBAND (BB) BEAM SPLITTER. .......... 164

FIGURE ‎6.19. RATIO OF THE TRANSMITTED RADIATION THROUGH SI SAMPLES WITH

AND WITHOUT GRAPHENE TO THE THE REFERENCE SPECTRUM WITH NO SAMPLE

IN THE BEAM PATH, WITH MCT DETECTOR AND KBR BEAM SPLITTER. .............. 164

FIGURE ‎6.20. RAW SPECTRUM OF THE TRANSMITTED RADIATION THROUGH PURE

GRAPHENE AND WITH NO SAMPLE, USING THE BOLOMETER AND BB. ................ 166

FIGURE ‎6.21. SPECTRUM OF THE TRANSMITTED RADIATION THROUGH PURE

GRAPHENE AND THE REFERENCE SPECTRUM WITH NO SAMPLE IN THE BEAM

PATH (INSET) USING FOURIER TRANSFORMS WITH BOLOMETER AND BB. .......... 166

FIGURE ‎6.22. RATIO OF THE TRANSMITTED SPECTRUM THROUGH PURE GRAPHENE TO

THE REFERENCE SPECTRUM WITH NO SAMPLE IN THE BEAM PATH, WITH

BOLOMETER AND BB. ........................................................................................ 167

FIGURE ‎6.23. RATIO OF THE TRANSMITTED SPECTRUM THROUGH PURE GRAPHENE TO

THE REFERENCE SPECTRUM WITH NO SAMPLE IN THE BEAM PATH, WITH MCT

DETECTOR AND KBR BEAM SPLITTER. ............................................................... 167

FIGURE ‎6.24. EXPERIMENTAL TRANSMISSION SPECTRA AND THE THEORETICAL

CURVE FITTING RESULTS FOR GRAPHENE ON SILICON AND SI ONLY. .................. 169

FIGURE ‎6.25. EXPERIMENTAL TRANSMISSION SPECTRA AND THE THEORETICAL

CURVE FITTING RESULTS FOR PURE GRAPHENE MULTILAYER. ............................ 171

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Chapter 1

1 Introduction to the Electronic and

Optical Properties of Graphene

1.1 Introduction

This introductory chapter first presents a background and literature review of

graphene and other types of carbon structure (Section 1.2). It then provides a detailed

study of graphene structuring from the chemical perspective (Section 1.3) before

explaining its physical properties (Section 1.4) including their most unique features of

the graphene structure (Section 1.4) of the monolayer and bilayer in zero-gap and

gapped graphene. This section discusses the most important physical theories that

describe the structure of graphene such as Bloch wave function and Tight binding

approach. Also, this section describes briefly the most important experimental studies

under the framework of this topic.

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1.2 Graphene: literature review and background

The graphene structure has been one of the most remarkable discoveries in

modern physics over the past 8 years, since 2004, when Andre Geim and his group at

the University of Manchester managed to isolate single layers of graphite, which are

called graphene. This discovery was a seminal event in the field of optoelectronic

materials, and it opened up a wide variety of theoretical and experimental research

work in the quantum physics field and in modern physics. Graphene, one of the

allotropes of carbon, is a one atom thick sheet of pure carbon, in which is the carbon

atoms are arranged in a honeycomb structure (hexagons). In 2010, Andre Geim and

Konstantin Novoselov were awarded the Nobel Prize for Physics for their "ground-

breaking experiments regarding the two-dimensional material graphene". This prize

was not just for the discovery of this material, but because they identified the unique

features of graphene that determine its optical and electronic properties.

In 1947 P. R. Wallace presented the first report on the unusual semiconducting

behaviour of graphite and explained the bond structure of graphite by using the new

theory of the tight binding model to explain the “superlattice” of bulk graphite [1].

There have been many reports since then describing the electronic properties of

graphite, which achieved convergence between theoretical and experimental results,

notably McClure (1957), and Slonczewski and Weiss (1958) [2,3]. After 1958, the

experimental work continued to yield data on the two-dimensional graphene layers of

this material, and these results were successfully interpreted by a number of

researchers such as Boylen and Nozieres (1958) [4], McClure (1958, 1964) [5], Soule

et al. (1964) [6], and others. P. R. Schroeder in 1968 provided new results on the

location of electrons and holes in graphene by using laser magneto-reflection data [7].

As a result of all these experiments and the characteristics that had been

discovered on the structuring of graphene sheets in graphite from 1947, it was

scientifically ground-breaking to study and achieve the desired goal of finding an

alternative material for the development of many optical and electronic devices. From

1954 to 1972, Linus Pauling succeeded in describing the allotrope of graphite, in his

quest into “The Nature of the Chemical Bond”, as consisting of layers of a “giant

molecule”, which we know today as graphite [8].

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A second type of carbon structure was discovered by Harold W. Kroto and

Richard E. Smalley in 1985, namely, fullerene "during experiments aimed at

understanding the mechanisms by which long-chain carbon molecules are formed in

interstellar space and circumstellar shells" [9]. They were honoured with the Nobel

Prize in Chemistry in 1996, and fullerene applications have been playing an important

role in all the natural sciences. Actually, in 1970, R. W. Henson was the first scientist

to publish a new report on the restructuring of carbon atoms in a football shaped

arrangement, but unfortunately, the evidence for this new type of carbon was very

weak and was not accepted. In 1991 Sumio Iijima discovered another member of the

fullerene structural family of carbon, an allotrope of carbon arranged in a giant

cylindrical molecule called the carbon nanotube, when he used an electron

microscope to examine carbon[10].

The van der Waals interactions between carbon atoms were used to explain many

phenomena that occur in graphene planes and in the carbon structures. In 2003 and

2004, Rydberg‟s group also reported on their use of the new method of many-body-

effects for direct evaluation of both the structure and the binding energy [11, 12].

Finally, considering carbon‟s role in the chain of life, it is very important to

understand the basic structure of graphene and know the electronic and optical

properties, as graphene is considered the mother for many types of carbon structures,

such as graphite, fullerenes, and carbon nanotubes.

In 2005, the Geim group, in collaboration with the Philip Kim group, achieved

an important finding, which contributed to the occurrence of another scientific

revolution in the field of graphene, that quasi-particles (the anomalous Hall Effect) in

graphene were unusual phenomena of two-dimensional massless Dirac fermions [13].

The Quantum Hall Effect (QHE) and Berry's phase in single graphene layers was

also reported by Zhang et al., who used high-mobility samples after failure to observe

the QHE in weak mobility samples [14]. As stated by Novoselov et al. (2007), the

Quantum Hall Effect (QHE) can be measured at room temperature (not just at liquid-

helium temperature) due to the large cyclotron energies for “relativistic” electrons

[15]. In fact, a Dirac fermion particle in graphene is moving at a speed 300 times

smaller than the speed of light at low energies, as the Fermi velocity, , which leads

to the many extraordinary properties of the QHE of graphene [16].

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In graphene, the most important findings were achieved experimentally, such as

the ballistic transport of electrons [17], the anomalous integer Quantum Hall effect

[16,13], weak localization, universal conductance, and the "Aharonov-Bohm effect

and broken valley degeneracy in graphene rings" [16,18].

Graphene is a gapless semiconductor, something that is very different from the

usual semiconductors, where the open gap between the conduction band and valence

band became the focus of much attention from scientists, In addition, many strategies

have been suggested to achieve a band gap in graphene [19,20]. There has been

success in theoretical and experimental research to find ways to open a gap between

the energy bands, but these ways are few and complex.

Furthermore, the nonlinear optical response in graphene and other kinds of

carbon structure can be strong in the terahertz regime in both interband [21] and

intraband transitions [22,23]. So, a strong nonlinear optical response in the visible and

infrared regime was reported by Refs. [24,25]. The light absorption of single layer

graphene has been reported theoretically [26] and confirmed by experimental [27]

results, and it was found that one layer of graphene absorbs 2.3 % of incident

infrared-to-visible light [28]. In 2009, the first ultra-short laser pulse work on

graphene samples was conducted [29,30]

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1.3 Carbon atom and structure of graphene from the

chemical viewpoint

The nature of chemical bonds, and the forms and shapes of structures are

responsible for determining most of the properties of materials. Consequently, we

have studied the electronic and optical properties of the element carbon and in various

forms and allotropes, but the most important studies relate to the two-dimensional

single layer of graphite which is known as graphene. Carbon is non-metallic and one

of the best known and most familiar materials for more than 400 years, when the

British first used carbon pencils for writing. It is the sixth element of the periodic

table and is the basis of all organic molecules. The electronic structure of one atom of

carbon is based on 6 electrons, i.e., , where represents the two

electrons near the nucleus, which occupy the inner orbitals and do not contribute to

chemical reactions. The four electrons ( ), however, which occupy the

external orbitals of the carbon atom are mixed together to contribute in three potential

types of hybridization ( ) in order to enhance the binding energy of the

carbon structure with near neighbouring atoms, forming the tight-bonded σ-bonds.

The fourth electron is associated with the bands, as shown in Fig. 1.1(a).

The angles of the hybridised orbitals are like the angles of an equilateral

triangle, as in Fig. 1(b). [31,32,33,34].

Carbon is the basis of all organic molecules. Pure carbon in the form of graphite

is made of single atomic layer thick crystals of hybridized atoms, which are

arranged in the two-dimensional honeycomb lattice structure of the carbon allotrope

called graphene (Fig. 1(c)) and tend to develop into other types of structure such as

graphite, fullerene, and nanotubes. Graphite is thus a three-dimensional (3D) structure

composed of a number of graphene layers of hexagonally structured carbon material.

In graphite, the graphene layers are weakly bonded to each other due to van der Waals

forces, with a distance between layers of about 3.35 Å [35]. It is graphene that

represents the basic building block for the graphitic structure. The structure of the

hexagonal lattice, with each hexagon defined by six carbon atoms, one in each corner,

is shown in Fig. 1(d).

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Figure ‎1.1 (a) Schematic representation of and bonds in graphene [28]; (b) schematic

view of hybridisation of carbon atom; (c) graphene is a carbon allotrope with a two-

dimensional honeycomb lattice structure; (d) typical hexagon from the graphene lattice

surrounded by six carbon atoms with one carbon atom in each corner.

C

C

(a) (b)

σ

σ

σ

(c)

0.142 nm

0.135 nm

Double bond C

C

C

C

C

C

(d)

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In addition, the carbon atoms are connected with each other by 6 covalent bonds:

there are 3 single bonds represented as C-C, and 3 double bonds lie between them and

are represented by C=C, with the distance between the atoms 0.147 nm and 0.135 nm

respectively [31].

Different layers of graphene may be stacked together and held by the weak van

der Waals covalent forces, to form a larger covalent structure, which is then called

graphite (Fig. 1.2(a)). Graphite may be a good conductor of electricity due to the vast

delocalization of electrons within the weak bonds in graphite, where the delocalized

electrons are free to move and are able to conduct electricity [31].

On the other hand, fullerene is another carbon allotrope; it is a zero dimensional

material, which has a similar composition to graphite but is made of hexagonal and

pentagonal structures joined together (in a design that resembles a football or soccer

ball (see Fig. 1.2(b)). Fullerene is produced by using an electric arc between two

graphite rods in a helium atmosphere to vaporize the carbon and takes the form of a

hollow sphere, ellipsoid, tube or ring. Fullerene remained in hiding until the late

twentieth century, unlike graphite and some other forms of carbon [33].

Carbon nanotubes (CNTs) are one of the most interesting materials due to their

unique physical properties, which have attracted the attention of scientists and

researchers since their discovery. They constitute a one-dimensional allotrope of

carbon and, consist of graphene sheets rolled up into cylindrical tubes with Nano-

scale diameters, as shown in Fig. 1.2(c). The electronic properties of the nanotube

depend on how the graphene sheet is rolled up [28]. Their thermal conductivity,

mechanical and electrical properties, and the strength of their sp² carbon bonds endow

CNTs with exciting mechanical, optical, and electronic properties and give them

significant potential for applications [36,37,38,39,40].

CNTs can be "metallic or semiconducting depending on their structural"

characteristics [41]. The first experiments with CNTs were conducted by using

Raman spectroscopy [41,42],where "Theoretical predictions for the dependence of the

transition energies on the nanotube diameter were used to narrow the possible

nanotube types in the sample" [41,43]. Resonant Raman spectroscopy was also very

important and useful for giving a description of the structure and electronic properties

of CNTs [41,42]. CNTs can be categorized in three structures as follows: Single-wall

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Nanotubes (SWNT) [44,45], Multi-wall Nanotubes (MWNT) [46], and Double-wall

Nanotubes (DWNT))[47,48].

Diamond is one of the oldest known carbon allotropes and was discovered in

India at least 3000 years ago. Diamond consists of a lattice of carbon atoms in the

form of a cubic structure (2-face-centred-cubic (2fcc)) of carbon atoms.. The well-

known diamond hardness is due to the strength of the connections between the

covalent bonds in the diamond structure, which is also characterized by high thermal

conductivity compared to other materials. The electronic structure of diamond is

based on hybridisation [49,50,31] (see Fig. 1.2(d)).

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Figure ‎1.2. (a) Lattice structure of graphite as graphene multilayer. (b) Fullerenes (C60)

are molecules consisting of wrapped graphene. (c) Carbon nanotube as a rolled up graphene

layer. (d) Unit cell of the diamond cubic crystal structure.

(b)

(a)

(c) (d)

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1.4 Geometry of the band structure of graphene's

honeycomb lattice from the physical viewpoint

The graphene structure has fascinating features, which is a good reason for

analysing it and studying its optical and electronic properties. The honeycomb

structure of graphene is made up of carbon atoms and takes the form of a hexagonal

configuration with two sublattices (2 carbon atoms per unit cell [16,51]), which can

be represented by two triangles in one lattice, as shown in Fig. 1.3(a). According to

this Figure, the graphene structure is not a Bravais lattice because two neighbouring

sites are not equivalent [31,52,32], but it is suitable to arrange a new triangular

Bravais lattice with two primitive sublattice vectors ( and ) as the A-A or B-B

sublattices, (see Fig. 1.3(a)), which are represented in the Cartesian x-y coordinate

system as follows :

( √ )

(1.1)

Where is the carbon-carbon distance of the bond length in the

graphene lattice. tIn addition, each point on the lattice of unit cells can be found by

using the real space graphene honeycomb lattice translation vectors [53]:

(1.2)

Where are two integers. Also, Fig. 3(a) shows the reciprocal lattice

with primitive unit vectors of hexagonal symmetry as

(

*

(

*

(1.3)

Where is the unit vector in the z direction, so, there are six points in the corner

of the graphene Brillion zone (see Fig. 3(b)), which contains two groups of in-

equivalent points (K and K'). These are called Dirac points [16,51] and are very

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important for describing the physical properties associated with the graphene

structure. Their positions can be expressed in this form:

(

√ *

(

√ *

(1.4)

The three nearest neighbour vectors which connect the A and B sublattices (A-B),

and hence the vectors for an A-sublattice atom are given by

( √ )

( √ )

while the vectors for a B- sublattice atom are the negatives of these.

Figure ‎1.3. (a): Graphene honeycomb lattice structure with the two graphene sublattices, and

primitive unit vectors and other unit cells as defined above. (b) Hexagonal structure of

graphene with reciprocal lattice vector and the first Brillouin zone.

𝐴 𝐵

𝑎 𝑎

𝛿

𝛿

𝛿

𝐴

𝐵

𝐵 𝐴

𝐴

𝐵 𝐴

𝐵 𝐵

𝐴

𝐵

𝑀

𝐾

𝐾 𝐾𝑋𝑦𝑦

𝑏

𝑏

𝐾𝑦𝑦𝑦

Γ

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1.4.1 Bloch wave function and tight binding approach

The unusual band structure of carbon monolayer sheets has been calculated

approximately by using one of the quantum mechanical approaches for solid material,

which is the tight binding model. This model describes the electronic properties of

graphene sheet between nearest neighbor carbon atoms in the honeycomb lattice and

includes only the state [32]. Theoretical studies based on the tight binding model

have provided significant analytical results and can be combined with experimental

studies, which will give good results. From 1928, Bloch succeeded in establishing the

first theory to explain the electronic states in a periodic crystal lattice, which

contributed to the building up of the wave functions of the electronic band structure.

The main problem in the tight-binding model, however, is to build a wave function

that is in the form of a combination of Bloch‟s wave functions for the two sublattices

(A-B sublattices), while maintaining the atomic structure [54,33]. In vibrational tight

binding, the total wave function for two atoms per unit cell can defined from the

Bloch wave functions by using Fourier transform analysis and can be written as

(1.5)

Here and are complex function coming from the A and B sublattices,

respectively, and

are the wave functions on the A and B sublattices,

respectively,and can be written in terms of the above-mentioned atomic wave

functions as

√ ∑

√ ∑

(1.6)

Where is the number of atoms in the honeycomb lattice, and are the real

atomic orbitals related to the orbitals in the two different atoms per unit cell, K is

the quasi-momentum, and and identify the locations of all atoms in A and B,

respectively. In addition, each sub-lattice atom in the graphene sheet is connected to

three nearest neighbors, and the angles between them are with respect to each

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other. Furthermore, to satisfy Bloch‟s theorem in terms of the atomic structure and to

describe the electronic band structure of the graphene monolayer, the total

wavefunction can be rewritten as follows:

( )

√ ∑

( )

(1.7)

Here, and is a Bravais lattice vector. The difference

between the two Bravais lattice vectors can be written in general form as follows:

( )

√ ∑ ( ) ( )

(1.8)

The band structure determining the graphene properties requires understanding

and calculating the time-independent Schrödinger‟s equation. Therefore, the solution

of this equation can be achieved by defining the Hamiltonian equation around each

point of the sublattice in the honeycomb structure, which participates in three (

and ) orbitals of the electronic band structure and may be written in matrix form

as a two-dimensional lattice [31,32]:

(

* (1.9)

Where the AA and AB terms represent the integrals between the orbitals of the A

atoms in the sublattice units and between the A and B sublattices, respectively, while

H is the Hamiltonian equation. In the absence of the two back scattering terms, the

Hamiltonian depends on two terms, and and can be rewritten in the form

below:

⟨ | |

⟨ | |

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Here and

include the two spinor components of the energy band.

The term is the approximate energy of the 2p orbital, and . The

solution of the overlap equation can easily be obtained from the matrix equation

(

) (

) (1.10)

Where

Then, from the overlap equation and by substitution into the characteristic

equation, we may obtain the eigenvalues of the Schrödinger equation, as follows:

[ ] (1.11)

describes the energy dispersion of the band structure, and it has two solutions,

i.e. two energy bands per unit cell as electron–hole symmetry, Therefore:

(1.12)

√ (

* (

) (

*

(1.13)

Where and are the components of the wave vector k at the corner of the

Brillion zone and is the nearest neighbor hopping energy of the graphene

honeycomb. The signs indicate the highest energy state within the valence

band and the lowest energy state within the conduction band, respectively. Figure

1.4(a) shows the electronic disposition and energy bands of the graphene monolayer

sheet in 3D, and Figure 1.4(b) shows a section of the energy band in 2D, which is

connected in two Dirac points, and all characteristic lines ( ).

Finally, to calculate the two components of the spinor wave function of the

Hamiltonian for monolayer graphene and solve the eigenfunctions around the corner

of the Brillouin zone (Dirac point), we can use the Schrödinger equation

, which may be rewritten in matrix form by substituting the Hamiltonian

equation and energy band structure in the graphene lattice as mentioned above, with

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multiplication of the Schrödinger equation by . The result can be written as

follows:

(1.14)

Then, the total wave function of the two atoms per unit cell, as shown in Figure

1.3(a), can be rewritten as

(1.15)

Where and are the two complex spinor components of the quasi-

momentum. Both of them are factors in the Bloch function as in the form below

∑ (

)

(1.16)

Finally, the Schrödinger equation for monolayer graphene, which includes all the

electronic characteristics and describes the electronic transitions in the honeycomb

structure, can be written in the following form:

(

)

(

) (1.17)

The first significant feature of this equation, which describes all photon processes

between the two energy bands (the valence and conduction bands) and around each

Dirac point in the monolayer graphene lattice, is that it also describes the electronic

transitions and important structure of this two-dimensional allotrope of carbon. This

equation gives good results in many cases and may be compared with other results,

such as experimental results or results from another theoretical model. Also, the use

of new methods in the various branches of quantum mechanics can achieve

substantial convergence with the results that have been presented and thus allow

access to new theories to explain the electronic and optical properties, such as the ab-

initio model. Therefore, the realization and control of the unique properties of

graphene material can open up new horizons in the field of optoelectronic devices.

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Figure ‎1.4. Energy dispersion in the honeycomb graphene lattice. (a) Left, the energy bands

of a graphene monolayer sheet in 3D. Right, the energy dispersion of graphene at the K-point,

which is known as the Dirac cone. (b) Comparison of ab-initio model and tight banding

model of graphene, showing good agreement at low energies [54].

(a)

(b)

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1.4.2 Single layer graphene

Graphene is a single-atomic-layer, two-dimensional system composed solely of

carbon atoms arranged in a hexagonal honeycomb lattice. It can be considered as the

basic building unit for other forms of carbon materials. Electronically, single layer

pure graphene is a zero band-gap semiconductor with two energy bands, the

conduction and valence bands, which meet at the Dirac point, as shown in Fig. 1.4(a)

(left). Only a brief account of the structure of the graphene monolayer will be given

here, because much of this has been already covered in detail, where the energy band

dispersion and wave function have been calculated by using a branch of quantum

mechanics, the tight-binding model, and also in terms of Bloch's theory in order to

satisfy the theoretical details. The energy dispersion approximation near the k and k'

points in graphene single layer can be rewritten as

| | (1.18)

Where is the Fermi velocity, and is the

hopping parameter. This energy around the k and k' points takes the shape of two

cones, where the one in the upper half of the dispersion is the conduction ( ) band

and the other one in the lower half is the valence ( ) band, with the two dispersions

touching each other at the zero energy point (Dirac point). Such an arrangement is

called a Dirac cone (see Fig. 1.4(a)). For the case of zero carrier density, the point

where the two bands cross the Fermi level coincides with the zero energy at the K and

K′ points of the first Brillouin zone, whose wave vectors are given by

√ √ and √ √ [55]. The effective low

energy Dirac Hamiltonian equation of two-dimensional single layer graphene

describes the charge carriers close to the Dirac point and also can be written as a 2 ×

2 square matrix, taking into account the relative Weyl fermion equation, as follows:

(

) (1.19)

Then, the Schrödinger equation can be revised in quite reasonable form by using

the Hamiltonian equation as above for spinless graphene carriers around the Dirac

point, which can be defined by

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Here, is the gradient with respect to the position (r), and is the operator of the

general Pauli matrices on the spinor which is expanded into two

dimensions, those of the x and y axes, and is given as

( ) (

)

(

) (

) (

) (1.20)

From these procedures, we reach the well-known Schrödinger equation of single

layer graphene, which will be reduced to the general form by modelling the

previously mentioned relations with the Dirac Hamiltonian equation around the K

point in the low energy system. Note that the particles behave as massless only around

this point, and the result therefore will be

(

) (

) (

)

This equation involves the two component spinors and describes a particle with

finite mass in the graphene lattice. It thus can be easily solved to yield the eigenvalues

and eigenfunctions, which are given by

√ (

*

√ (

*

(1.21)

Here, indicates the K and K' valley, respectively, and

is defined by the direction of the wave vector in k space [16,33,51,54].

The rotation of in both the and the planes by , will result in a change in

phase by , with the new phase called a Berry's phase. That change in phase by is

one feature that describes the two spinors of the wave function.

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1.4.2.1 The electronic structure of gapped single layer graphene

All the above discussion describes the electronic structure of single layer

graphene under gapless (zero band-gap) conditions, so it is important to address

another form of the energy bands, that is, a gap between the energy bands at the Dirac

point. The arrangement of the two sub-lattices of carbon atoms is responsible for the

zero energy between the bands. Consequently, a breaking of the symmetry between

the A and B sub-lattices at the Dirac point would cause a gap to open up [56].

Furthermore, the possible ways to break the symmetry and to open up the gap include,

for example, strain engineering [57, 58], graphene-substrate interaction [59,60],

confinement [61], and chemical modification of graphene [62]. The absence of the

energy gap in graphene blocks the development of many optical and electronic

applications.

So, we will follow the same steps as in the gapless case to calculate the

eigenvalues and eigenfunctions with a band gap, and then the Hamiltonian equation

around the k point at low energy can be written in the form below:

(

, (1.22)

Here, and represent the energy bands at the Dirac point.

The eigenvalue is given by substituting the Hamiltonian equation for the energy

gap condition into the characteristic equation as follows:

√ | | √

(1.23)

The equation above describes the energy spectrum around the K point below the

band gap. In addition, with an energy gap in single layer graphene, there is the clear

fact that the charge carrier has a finite mass, so that the behaviour of this energy

equation is not linear in the low energy regime, but on the other hand, the behaviour

of the electrons cannot be obtained without destroying the linear behaviour and

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breaking the symmetry of the graphene single layer structure [63]. In addition, the

wave function for two compound spinors in this system can be calculated by

substituting the Hamiltonian matrix as above into the Schrödinger equation and is

given as follows [56]:

√ (

( )

√| |

| | ( )

, (1.24)

The density of states for gapped graphene can be defined by

| |

(| | )

(1.25)

Where and are the degrees of freedom associated with the spin

and the valley, respectively, and is a step function [63, 64]. Finally, to control the

semiconducting properties and tune the Fermi level of graphene, we can use doping,

chemical modification, and electrostatic field tuning [65].

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1.4.2.2 The experimental work of Single layer graphene

The discussion above is concerned with the theoretical expression of the

graphene structure in two forms, with and without a band gap. So, it is worthwhile to

compare the theoretical results with the experimental results to achieve a

comprehensive understanding of the electronic structure of the honeycomb lattice of

carbon atoms in 2D. Therefore, in this section we will address briefly the most

important experimental studies under the framework of this topic. Since the isolation

of single layers of graphite in 2004 [66], several exciting experimental studies on

single layer graphene have been conducted. In addition, a number of efforts were

combined from 1990 to 2004 to attempt fabrication of thin films of graphite.

Unfortunately, these attempts did not succeed, however, except in obtaining films

several tens of layers thick, amounting to about 50 to 100 layers until 2004, when a

group of scientists succeeded (the first experimental establishment) in the fabrication

of single-atom-thick two-dimensional graphene crystalline material [67] (as shown in

Fig. 1.5(a-d)). After that, these isolated samples were taken and placed over a thin

layer of SiO2 on a silicon wafer. The layer of Si under the SiO2 was used as a "back

gate" electrode to change the charge density in the honeycomb lattice over a wide

range [68]. The first observation of the unique properties of graphene by using the

micromechanical cleavage technique was of the Anomalous Quantum Hall Effect.

That validated the theoretical results and predicted a -shifted Berry's phase of

massless Dirac fermions in graphene [69]. Recently, monolayer graphene films have

been achieved by chemical vapour deposition on a thin substrate of nickel layers and

silicon wafer covered by a layer of silicon oxide. In addition, this offered different

methods of modelling the films for the synthesis of large-scale graphene films

[70,71], which have provided a clear explanation of the typical Quantum Hall Effect

for single layer graphene. As has proved important, using monolayer graphene films

is better than multilayered due to their higher trans-conductance and optical

transparency [71,72]. "Hence, epitaxial graphene reproduces the unique features

observed in exfoliated graphene, but is certainly a system which allows for more

systematic development of graphene devices, with rich perspectives for science and

technology" [72].

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Figure ‎1.5. Optical microscope image of a graphene flake: (a) Three regions can be

identified: I, single-layer graphene; II, multilayer graphene; and III, the silicon-dioxide-coated

substrate. (b) Image of the same flake after the deposition of an 18-nm layer of gold. (c) STM

image of a single-layer graphene film on the silicon dioxide surface. (d) The full hexagonal

symmetry expected of an isolated single layer graphene sheet. (e) Image of the multilayer

portion of the sample [68].

d e

c

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1.4.2.3 Single layer graphene Nano-ribbons

Understanding the electronic structure of the graphene honeycomb requires a

microscopic view to fully elucidate the structure of the carbon constituents. Their

electronic structure actually remained unknown for a long time until K. Nakada et al.

was able to provide a study of nanometre-scale graphite networks by using the model

of graphene ribbons with various edge shapes, which also provided mathematical

details on the features of the states at the edge and the localized states close to the

Fermi level in the honeycomb structure with zigzag and armchair edge functions [73].

Hence, studying graphene nanoribbons and their surface (edges) is a very significant

and plays an effective role in determining the characteristics of graphene. There are

two types of edges that represent the final borders, or semifinal in the graphene sheet,

and these are the zigzag and armchair edges as shown in Fig. 1.6(a, b).

The nature of the edges in the graphene sheet is responsible for the spectrum and

the structural axis of graphene sheets. As shown in Fig. 1.6(a) the zigzag edges are

represented along the x-axis, whereas the armchair edges are represented along the y-

axis. The nanoribbons of graphene can described by narrow rectangles made from the

honeycomb structure, which have widths up to 10 nanometres, and are therefore

classified under the category of nanoscale materials, These can possess the

characteristics of a semiconductor, which gives us an opportunity to study their

optical and electronic properties due to the significant changes in these properties

from quantization. Theoretically, the calculations of the general band structure of the

graphene nanoribbons (GNR) are obtained from the Hamiltonian equation by using

wave mechanics based on the tight-binding model or some other method [74].

"The energy band structures of armchair nanoribbons can be obtained by making

the transverse wavenumber discrete, in accordance with the edge boundary condition,

as in the case of carbon nanotubes. However, zigzag nanoribbons are not analogous to

carbon nanotubes, because in zigzag nanoribbons, the transverse wavenumber

depends not only on the ribbon width, but also on the longitudinal wavenumber."

[75].

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Figure ‎1.6. The finite-width honeycomb structure of graphene nanoribbons: (a) zigzag edge of

graphene nanoribbons; (b) armchair edge of graphene nanoribbons.

The Dirac Hamiltonian equation of the GNR band structure around the K and K'

points is calculated as described previously for the general band structure of the

graphene honeycomb. The spinor wave function of GNR can obtained, however, by

assuming that the edge of the graphene sheet is parallel to the x direction as in a

zigzag nanoribbon (see Fig. 1.6(a)) and to the y direction as in an armchair

nanoribbon (see Fig. 1.6(b)), which can be expressed by

(

*

(

*

The boundary condition of the GNR at the zigzag edge and armchair edge can be

provided as follows:

Here, is the ribbon width. Under these conditions and to satisfy the Bloch

theorem, the two compound spinor wave function can be rewritten from the envelope

function as follows:

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Then, by following a similar method to that used to calculate the eigenvalues, the

eigenfunctions and the band structure of general pure graphene can be found by using

the Schrödinger equation [16,51]. The energy dispersion spectrum for armchair and

zigzag nanoribbons is given respectively by [75]:

√ (

*

√ ( (

**

(

*

(1.26)

The energy gap plays an important role, which is related to the width of the edge

of the graphene ribbon, where the energy gap for zigzag ribbons (at ) and the

energy gap for armchair ribbons (at ) increases as a result of a decrease in

the width of the graphene ribbons [75]. The great challenge, however, remains control

of the energy gap. Finally, to achieve a really good description of the graphene

nanoribbon, it is necessary to know the number of armchair (a) and zigzag (z) chains

that are present in the length and width directions, as shown in Fig. 1.6(a, b), which

shows "how to count the number of chains for a 9-aGNR and a 6-zGNR. The width of

the GNRs can be expressed in terms of the number of lateral chains" [54]:

(1.27)

Here is the lattice constant of the honeycomb lattice. The lengths of

the primitive unit cells are √ and for armchair and zigzag nanoribbons,

respectively. Numerical calculations are used to calculate the band structure of the

graphene nanoribbons and are based on the first principles of the intrinsic graphene

and the tight binding approximation, which is described in the previous section. All

these features mentioned above may lead to the development of electronic devices.

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1.4.3 Bilayer graphene

The isolation of individual graphene flakes in 2D by using mechanical exfoliation

was one of the biggest events in the world of modern physics. Hence, a

comprehensive review has been provided in the above sections of studies of

monolayer graphene, which has been the subject of great attention and attracted

scientists to study its unique characteristics. Here, we will review a brief study of two

stacked layers of graphene, called bilayer graphene, which is believed to exhibit more

important features than the single layer due to the Anomalous Integral

Quantum Hall Effect (IQHE) [76, 77, 78], and also provides a greater opportunity to

open a tunable gap between the band energies [79,80,81,82,83] and to examine the

trigonal warping phenomenon [84,85].

The tight-binding model for graphite can be easily be extended to bilayer

graphene by using the theoretical study of single layer graphene and developing the

Hamiltonian equation to involve the electronic transitions between the two layers,

which is needed to understand the binding energy for both layers. Taking into

account the four atoms per unit cell, there are two sublattices A and B for each layer,

as shown in Fig. 1.7(a,b). The Hamiltonian equation for the nearest neighbors labeled

as ( under low energy and around the k point, can be obtained by

(

, (1.28)

Where , , , are the parameters of plane hopping between the two layers

and can be defined by [86]

⟨ | | ⟩ ⟨ | | ⟩

⟨ | | ⟩

⟨ | | ⟩

⟨ | | ⟩ ⟨ | | ⟩

The function f(k) represents nearest-neighbor hopping and is written as follows:

√ √ (1.29)

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The Hamiltonian matrix presented above can be described accurately by splitting

it into four regions; the upper-right and lower-left 2 × 2 squares represent the

interlayer coupling. Factor is the coupling between orbitals on sites B1 and A2, and

factor is the interlayer coupling between orbitals A1 and B2. Factor is the

interlayer coupling between orbitals A1 and A2 or B1 and B2. On the other hand, the

upper-left and lower-right 2 × 2 squares represent the intralayer coupling and also

represent a description of the transitions that occur in the monolayer. In addition, the

parameters , , and describe the energies of bilayer graphene on sites

, , and respectively. Here, the factor represents the

nearest-neighbor hopping energy within a single layer [86,87] and

( ) where is the velocity.

Figure ‎1.7. (a) Schematic diagram of lattice structure of bilayer graphene in (a) a plane

and (b) a side view of the crystal structure [86]. (c) Schematic of low energy bands around K

points.

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The overlap integral equation for bilayer graphene can be written in matrix form:

(

, (1.30)

This equation mirrors . Where ⟨ | ⟩ ⟨ | ⟩ describing the

orthogonally of orbitals on sites A1 and B1 or A2 and B2. Also, ⟨ | ⟩

⟨ | ⟩ describing the orthogonality of orbitals on sites A1 and B2 or A2 and B1.

From the Hamiltonian equation, four energy bands can be obtained, as shown in Fig.

1.7(c) and substituted into the characteristic equation as follows [86]:

Where

[ ],

[ ]

and

[ ]. Under the tight-binding model, the Bloch

function of the bilayer graphene wave function can be obtained by substituting into

the Schrödinger equation to obtain the four solutions of the wave function, as [88]:

√ ∑ ( ) ( )

√ ∑ ( ) ( )

√ ∑ ( ) ( )

√ ∑ ( ) ( )

Here, is the lattice vector, N is the number of unit cells, and the vectors and

represent the links between the nearest atoms in the same layer and the nearest

atoms in the neighbouring layer, respectively. Basically, electrons in bilayers behave

qualitatively differently than in single layers. The low energy bilayer graphene

(BLG) exists in different forms, depending on the coupling terms between the layers,

so it is important to know the nature of the coupling to determine the form of the

electronic band structure and move forward to calculate the eigenvalues, the

eigenfunctions, and the energy band structure.

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1.5 Scope of thesis

The aim of this thesis is to provide a study of the optical and electronic properties

of the graphene structure in two parts, theoretical and experimental. The first chapter

presents the background and a literature review of the graphene structure in the

context of other types of carbon structure. It provides a detailed study of the graphene

structure from the chemical and physical viewpoint and explains the most unique

features that characterize it. The graphene structure is calculated for monolayers and

bilayers in zero-gap and gapped graphene.

The second chapter of this thesis presents the calculation and analysis of the

strong nonlinear optical response in the terahertz to infrared regime in monolayer

gapless and gapped graphene p-n junctions under moderate electric field. By using the

Boltzmann transport equation, the linear and nonlinear optical conductivity can be

described, with and without a band gap, in relation to the intraband transitions. Then,

the tight binding model is considered with and without band gap. Additionally, an

analysis is provided of the quantum mechanical approach in order to calculate the

linear and nonlinear conductivity of interband transitions. Finally, the total intraband

and interband conductivity of single layer graphene can be calculated.

The third chapter of this thesis discusses the photon mixing linear and nonlinear

response, taking into consideration the full temperature spectrum of the nonlinear

optical response of a finite-doped ( ) graphene single layer in both the gapless

and the gapped cases under both weak-field and strong-field conditions in the

terahertz to infrared regime.

The fourth chapter of this thesis presents the linear and nonlinear optical response

of bilayer graphene in the terahertz to infrared frequency regime. Under moderate

electric field intensity, the quantum mechanical approach treats the coupling of Dirac

electrons to the time dependent electric field quantum mechanically to calculate the

strong nonlinear term in the multiple photon case. Also, the required field strength to

induce a non-negligible nonlinear effect is determined. In the second, third and fourth

chapters, the theoretical approach is used to calculate the linear and non-linear optical

response by using a quantum mechanical model.

The fifth chapter of this thesis provides a full explanation of the samples and the

devices used in the laboratory and the most important features that characterize these

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devices, such as the Fourier transform spectrometer and detector used to measure

absorbance and transmittance. An explanation of the programs and calculations used

for data and graphic analysis is also provided.

The sixth chapter of this thesis presents a study of the transmittance and

absorption spectra of graphene, silicon coated by graphene. The effects of electric

field on the samples are determined by applying voltage on the sample at different

temperatures to measure the output current. Secondly, the effects of temperature on

the peak of absorbance and transmittance of graphene with and without silicon

substrate are also confirmed. Particular emphasis is given to the effects of an infrared

beam on the transmittance and absorption spectra in different samples and under

different conditions.

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Chapter 2

2 Nonlinear Optical Conductance of a

Single layer Graphene p-n Junction in

the Terahertz Regime

2.1 Introduction

The optical conductance of graphene based systems in the terahertz to far infrared

regime has been a topic of intense interest due to the ongoing search for viable

terahertz detectors and emitters. In addition, there are many theoretical and

experimental reports on this topic, and results suggest that graphene can be used for

building innovative devices for terahertz optoelectronics. Furthermore, graphene is

gapless semiconductor, and it has a very good conductivity, better than silicon It has a

strong nonlinear response in the terahertz regime. Moreover, the nonlinear strong

response has been reported in many research works using a quantum mechanical

approach [21, 89, 90].

The p-n junction is the basic building block for electronic devices, and it is very

significant for developing graphene based THz radiation sources and other application

devices. In graphene p-n junctions, for a symmetric p (hole) − n (electron) junction

[91], the transition from the conduction band (n-type layer) to the valence band (p-

type layer) represents dynamic changes from the electron to the hole band, as shown

in Fig. 2.1. Generally in this case, the electrons have left the conduction band

(positive region) and passed into the valence band (negative region) due to electron

diffusion. Also, the electron band and hole band meet each other at the Dirac point.

The main purpose of this Chapter is to calculate and analyse the strong nonlinear

optical response in the terahertz to infrared regime in monolayer gapless and gaped

graphene p-n junctions under moderate electric field. By using the Boltzmann

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transport equation, we study the linear and nonlinear optical conductivity due to

intraband transitions in junctions with and without band gaps. Then, we describe the

tight binding model with and without a band gap. Additionally, we use the quantum

mechanical approach to calculate the linear and nonlinear conductivity of interband

transitions. Finally, we calculate the sum of intraband and interband conductivity for

single layer graphene.

Figure ‎2.1. Schematic diagram of the band structure of graphene p-n junction. (a) illustrates

the dual gate voltage of graphene in the p-n junction regime [92]. (b) Energy band diagram of

single layer gapless graphene with bias voltage in both sides ( p region and n region).

2.2 Single layer gapless graphene p-n junction

Single-layer graphene (SLG) is a gapless two-dimensional semimetal and has an

uncomplicated band structure, but the optical response and high conductance of

graphene between the n region and the p region may result in many features of the

electronic transitions.

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In this section, a single layer graphene based structure will be considered with a

substrate layer 300 nm in thickness with split gates . The gate voltages

and are applied over the p region and the n region, respectively, with a forward

bias voltage between both regions. The Fermi energy can be obtained from the

sheet density, where the carrier sheet density is [92, 93, 13].

Figure 2.1(a) and (b) shows the schematic band structure of single layer gapless

graphene in the p-n junction regime with moderate electric field. In addition, the

Fermi energy can be calculated by using the gate voltage as follows [92, 94]

(2.1)

where . is the thickness of the gate layer, and p is

momentum. The concentrations of electrons and holes can be controlled by using the

gate voltage, which defines the density of electrons (p+ region) and holes (n

- region)

in graphene and is related to the Fermi energy or chemical potential in the form below

[92, 94, 95]

(

*

(2.2)

where and are the density of electron and holes, respectively, and and

are the Fermi energies of the conduction band and the valence band electrons

[96]. and represent the Fermi distribution function for electrons and holes,

respectively, which can be written as follows

(

*

[ (

*

(

*]

(2.3)

The energy is where the Fermi velocity for electrons and holes

is . In the equations above, the charge carriers are thermally excited to the

conduction or valence band of graphene, and in addition, n = p and in

the graphene layers [96].

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2.1.1 Intraband Transitions

In this section we employ the Boltzmann equation to calculate the optical

conductivity of the intraband transitions of the SLG p-n junction under electric field

along the x-axis , where time dependent :

(2.4)

Where and are the equilibrium and non-equilibrium distribution function,

respectively, and is the momentum scattering time. Introducing and

substituting

in Eq. (2.4), we obtain

(

*

Then we obtain

(2.5)

Where , the corresponding current density is written as

(2.6)

Where with the Fermi velocity and

(

) . The order optical conductivity with intraband transitions

can be written in the form of:

∫ (

*

(2.7)

We now calculate the real part of the optical conductivity, which is defined as

optical conductance. The linear optical conductance associated with intraband

transitions is given as

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∫ (

*

(2.8)

By substituting n = 2, we obtain the second order optical conductivity associated

with the intraband transition. As expected due to the time reversal

symmetry. The third order n = 3 conductance associated with the intraband transition

can be written as

[ ]

∫ (

)

(2.9)

Where ( ) [ ( ) ]

, and represent the

Boltzmann constant and the temperature respectively. Numerical calculations can be

used to solve the third order nonlinear optical conductance with intraband transitions

(electron and photon scattering processes) when . At zero temperature

will go to infinity. On the other hand, we assumed the limits of integration in

Equations (2.8) and (2.9) can be cut-off at a large Fermi level between 0 (lower limit)

and 0.5 eV (upper limit) to avoid the infinity in integration. The equation above is the

expression for the absorbed energy due to transition between quantized levels [95]

Finally, we studied the linear and nonlinear conductivity due to intraband

transitions between the quantized levels in single layer gapless graphene p-n junction

in the conduction or valence band in the infrared to THz regime. The optical intraband

transitions in monolayer and few layer graphene have been reported for many

theoretical and experimental investigations [96, 92, 97, 98].

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2.1.2 Inter band transitions

The interband transitions are important for optical projects, and there are several

interesting features that can be observed with respect to interband transitions in

monolayer graphene. The interband transitions are quite strong.

In this section, we calculate the optical interband transitions by the tight binding

Hamiltonian as a quantum mechanical approach. Under low-energy and non-

equilibrium conditions for the zero-gap single-layer graphene p-n junction, we obtain

(

*

(2.11)

Where and

. The wave function can be expanded into

two spinor two spinner components in the basis set as follows

∑ [

] ( )

(2.11)

Where the eigenvalue is | | , and and are two component

spinors that represent the wave function in the two sublattices in single layer

graphene, where the Hamiltonian is a 2 × 2 matrix. The signs + and – refer to the two

energy bands (conduction and valence band). By substituting the wave function and

Hamiltonian equation into the Schrödinger equation , we obtain

(

* (

) ∑

(

)∑

(

* (

) ∑

(

)∑

From the above equation, we can write the coupled recursion relation for the

spinor components due to the orthonormal relations of .

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( )(

( ) )

( )(

( ) )

(2.12)

The and describe all the photon processes in the electronic states of the

graphene structure in thje order when . The terms and are

operative when the electric field is greater than zero. If the electric field = 0, only n =

0 terms are nonzero, and the solution to Eq. (2.12) is similar to the general massless

Dirac fermion wave function. In this case, the normalization of the wave function in

zero order can be defined as

(

)

√ (

+

(2.13)

From Eq. (2.11), we can calculate the order linear and nonlinear current and

conductance. Now let us calculate Eq. (2.12) when n = 1, 2, 3.

First order, when n = 1, to solve Equation (2.11) where there is , we obtain

( )( ( ) )

( )(

( )

√ )

( )(

) (2.14)

And the solving for , we obtain

( )( ( ) )

( )( ( ) )

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( )( )

(2.15)

Second order n = 2

In the second order of the equation (2.11) to solve for , we have

( )( ( ) )

( )( )( (

)

( )( ))

( )( )( *

[ ]+

( )*

(2.16)

The solution of :

( )( ( ) )

( )( )(

[

]

)

( )( )(

[

] [

])

(2.17)

Third order n = 3

( )( ( ) )

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39

( )( )( )(

[ ]

( ) (

){ [

] [

]})

assuming that

( )( )( ) will be reduced to

the form of

(

{ ( )}

[ ]

( ){ [

] [

]})

(2.18)

Finally, we have to solve the third order when

( )( ( ) )

( [

]

( )[

( ) (

)])

(2.19)

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2.1.2.1 Linear conductivity

The general form of linear and nonlinear current in the order is given by

∫ , where [ ( )]

[ ( )]

is the thermal factor, is the current operator,

where

and is the forward bias voltage. By using the general current

equation and the solution of Eq. (2.12), we can proceed to calculate the real part of the

order optical conductivity associated with an intraband transition under moderate

electric field, which is defined as follows:

( ∑

+

(2.21)

Where n = 1

(2.21)

By substituting Eq.(2.21) into Eq. (2.20), we obtain the optical conductivity for

n=1,

∫ ( ∑

+

We can expand into two parts, depending on Equation (2.44), as follows,

∫ ( ∑

+

(2.23)

and

∫ (∑

+

(2.24)

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Then, we sum over the two terms above to arrive at the linear optical

conductivity, as in the following equation,

Now we are going to find the first part

of the optical conductivity, when

, so we rewrite the equation above as

( )(

)

( )(

)

(

) ( )

*

(

)+

(

*

(

*

[ (

* (

*]

(2.25)

where [ ( )]

is distribution function of the p-n

junction. is the forward bias voltage, is the Fermi energy, and the temperature.

By using the same method, we can obtaine the second part

. Finally, the first

order optical conductivity is given by

(

*

(

*

[ (

* (

*]

(2.26)

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In our results, the calculations of the optical conductivity and the current with the

n = 1 term are equivalent to the linear response result. The total linear optical

conductivity is the sum of intraband and interband linear terms oscillating with

frequency .

(2.27)

From Eq. (2.27), we plot the total linear optical conductance of the single-layer

gapless graphene p-n junction oscillating with frequency in units of with

different values of the relaxation time . When the Fermi energy is 24 meV ( =

18.56 V), the bias voltage is = 40 mV and T =7 7 K, there exists a frequency region

of where the conductance is negative. The negative conductance is due to

the interband transition. From Eq. (2.27), will be negative under the

condition . When , will be negative in the range of

frequencies below 10 THz. In other words, the sums of the linear optical

conductivities

and

are negative in some part of the terahertz regime,

as shown in Fig. 2.2. Furthermore, the linear negative conductivity of the p-n junction

increases with increasing the relaxation time. However, we found that when the

frequency increases, the relaxation time will have a negligible effect on the linear

optical conductivity. From this we can conclude that the linear optical conductivity

effect of (intra-band transition) will diminish with the frequency increasing due to the

weak transition between quantized levels. On the other hand, the second order optical

conductivity associated with interband transitions

is also zero because of

time-reversal symmetry, which means that the total second order optical conductivity

will be zero.

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43

Figure ‎2.2. The total real part of the linear optical conductance of a single-layer gapless

graphene p-n junction oscillating with frequency in unit of with different values of

the relaxation time when and at T = 77K.

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44

2.1.2.2 Nonlinear conductivity

In this section, the real part of the third order optical conductivity of the single

layer gapless graphene p-n junction that is associated with intraband transition can be

calculated by expanding Eq. (2.20) to the third order and using the following formula

( ∑

+

(2.28)

To calculate the third order optical conductivity we will consider the current

operator term in the following form

(2.29)

Then, we have two terms of the third order conductivity, where the first term is

the single frequency and second term is the the triple frequency

. This

can be used in rewriting tEq. (2.28) as:

∫ ( ∑

+

(2.31)

∫ ( ∑

+

(2.31)

By using the same method for the linear term, we can solve the third order single

frequency term by substituting Eqs. (2.14), (2.15), (2.16), and (2.17) into Eq. (2.30).

We will distribute Eq. (2.30) into two terms. The first term can be expressed by

∫ (∑

+

( )( )( )(

) ( *

[ ]+ ( )*

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when the integration of ∫

, due to

For those conditions, the single frequency of third order conductivity can be

rewritten as

∫ (∑

+

( ) ( )

[

]

∫ (∑

+

[

( ) ] (

)

Then,

∫ ∑

*

+

∫ (∑

+

|

(2.32)

Then, we solve the second term of the single frequency nonlinear part of Eq.

when the integration over all .

∫ ( ∑

+

( )( ) [

]

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∫ ( ∑

+

[

]

( ) (

)

∫ ( ∑

+

|

(2.33)

Finally, we sum the two terms of by substituting Eqs. (2.32) and (2.33)

into Eq. 2.28. One can write

(2.34)

Considering Equation (2.31), one can determine the third order conductivity at

triple frequency by substitute Eqs. (2.13), (2.18), and (2.19) into Eq. (2.31).

Firstly we will expand equation (2.31) in two terms to make it easy to solve. So, we

have to consider the first term of the triple frequency nonlinear optical conductivity

when , as follows

√ (

( )

( ){ [ ]

})

where

( )( )( ). So, we have

∫ ∫

√ (

( ) ( ){

})

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47

The second term of the triple frequency nonlinear optical conductivity can be

simply shown to be

√ ( [

] ( )[

( ) ( )( )])

So we have,

√ (

( ) ( )[

])

Finally, to procede to the the third order conductivity at triple frequency

with interband transitions, we will consider the two terms of and substitute

them into Eq. (2.31). So, we rewrite Equation (2.31) as

( )( )( )(

)

(

) *

( )

( )( )

( )

( )( )

( )

( )( )+

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48

(

) *

( )

( )( )

( )

( )( )

( )

( )( )+

So, that can be written as

*

(

)

(

)

(

*

(

)

( ) (

)

(

*+

Finally, the equation will be reduced to the form of

[

(

*

(

*]

(2.35)

After calculation and analysis of the third order nonlinear optical conductivity in

two terms,

associated with interband transitions, we have to

calculate the total third order nonlinear optical conductivity . Summing

as represented in Eq. (2.34) and Eq. (2.35), respectively, in Eq.

(2.28), we arrive at the following equation

[ ]

(2.36)

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49

Where

(

(

*

(

*+

.

So, the terms proportional to correspond to the process of simultaneous

absorption of three photons, and corresponds to process of absorption of two

photons and immediately emitting one photon.

In Fig. 2.3 we plot the total linear and nonlinear (intra- and inter) band

conductance of a graphene p-n junction in a zero gap band under a moderate field as a

function of frequency vs. the relaxation time when the Fermi energy is 24 meV, the

bias voltage 40 mV, and the relaxation time 10 ps for different electric field

intensities. In this Figure, we can observe that when the frequency increases below

approximately 4 THz and , the rate of change in the electric field will

have a negligible effect on the nonlinear optical conductivity. However, we found that

The third order optical conductivity of intra-band and inter-band are changed by the

high field because of the (intra- and inter)transition. The nonlinear process can be

negligible by the weak electric field.

Furthermore, the nonlinear negative conductivity can be enhanced by using an

external electric field. Figure 2.4 shows the electric field dependence of the ratio of

nonlinear to linear optical conductance at different frequencies. Note that the

nonlinear conductance is larger than the linear conductance when the electric field

intensity is around . At moderate field strength, the real part of the total

optical conductivity is negative over a very wide frequency range covering the entire

terahertz regime.

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50

Figure ‎2.3. The real part of the total optical conductivity of the graphene p-n junction as a

function of frequency for different electric field intensity, with τ = 10 ps, meV, and

bias voltage .

Figure ‎2.4. The ratio of the real part of the nonlinear and linear optical conductivity vs. the

electric field intensity, with , bias voltage and the .

Rat

io o

f N

onli

nea

r &

lin

ear

Op

t. c

ond

ctiv

ity

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51

2.3 Single-layer gapped graphene p-n junction

This section presents a study of the optical conductance of a single-layer gapped

graphene p-n junction associated with intraband and interband transitions. The optical

conductance of gapped graphene provides significant information for studying optical

properties and electron transitions between the energy bands, and that can be useful

for developing graphene-based optical devices. In addition, opening a gap at the Dirac

point has become a necessity for many electronic applications. Furthermore, the

absence of the gap in graphene can be an obstacle to other electronics application.

Graphene p-n junctions can play an important role in developing tunable THz

radiation sources and other devices. Graphene with a gap exhibits an interesting

optical response at low frequencies [99]. Figure 2.5 is a schematic diagram describing

the transfer of electrons from the p-region to the n-region in single-layer gapped

graphene in a p-n junction regime.

In gapped graphene p-n junctions, the electrons move from the electron to

the hole band with a band gap at the Dirac point due to electron diffusion under bias

voltage, and the carriers redistribute themselves in such a way as to equalize the

Fermi level throughout graphene band, and electric field is applied to control the

band-gap size. On the other hand, building in dual gate voltage on both sides (p-

region) and (n-region) can control the Fermi level of graphene, but the band

gap cannot be opened [65].

The opening of an energy band gap in SLG has been observed due to

breaking the symmetry between the A and B sublattices. It was recently reported,

however, that a band gap can be produced in SLG between the conduction and

valence bands by adjustment of combined 1D electrical and magnetic fields [100].

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52

Figure ‎2.5. Schematic diagram of the band structure of gapped single-layer graphene in the p-

n junction regime under moderate electric field.

2.3.1 Intraband Transitions

To calculate and analyse the linear and nonlinear optical response associated with

intraband transitions between the quantized levels in a gapped graphene p-n junction

will be require the same equations that are used for any gapless graphene. There is no

effect of the gap on the electron transfer (intraband) between the quantized levels.

From Eq.s (2.7), (2.8), and Eq. (2.9), the linear and nonlinear conductance associated

with intraband transition can be calculated.

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53

2.3.2 Interband Transitions

Here, we demonstrate the optical response associated with interband transitions

of a single-layer gapped graphene p-n junction by using the tight binding Hamiltonian

in the low energy regime, so the Hamiltonian matrix between the A and B sublattices

with a band gap is defined as:

(

)

(2.37)

where and are the energy gaps between the middle of the band gap

and the conduction band and valence band, respectively. From the Hamiltonian

equation, the eigenvalues in zero applied field acan be found:

(2.38)

where s = ±1. By substituting the Hamiltonian equation and eigenstates into the

Schrödinger equation, as in previous work, we can obtain the following results

The left side of Schrödinger equation, can be expressed by

(

,(

) ∑

So, for the right side of the Schrödinger equation, one can write

(

)∑

Then, we can make some mathematical rearrangements on the left and right hand

sides of the Schrödinger equation, and these equations can be expressed by

(

)(

) (

)

(2.39)

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54

From Eq. (2.39), we can write the coupled recursion for the spinor components

due to the orthonormal relations of with the band gap in the following form:

( )

( )

( )

(2.40)

From the solution of Eq. (2.40), we can calculate the order current,

∫ where [ ] and

[ ( ) ]

is the Fermi-Dirac distribution function of

the electrons and holes in the n and p regions [11], and the velocity operator

.

When the electric field is zero the wave function can be written as

(

+ (2.41)

Now, we proceed to find the solution of Eq. (2.40) for the order for n = 1, 2,

3, which can help us to solve the optical conductivity, so that we obtain the solution

for the two spinor components as follows

( )

(

)

(2.42)

Then

( )

(

*

( )

(

* (2.43)

So, for the second order when n = 2, we have

( )

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55

(

)√

(

(

*)

(2.44)

and

( )

( )

( )(

)√

(

)

(2.45)

Finally, we have to calculate the third order when n = 3, so the solution will be in

the form of

( )

( )

(

)

(2.46)

where ( )

( ),

( )

( )

(

(

)

(

*)

(2.47)

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56

2.3.3 Linear conductivity

Under conditions of the THz regime and T ≥ 0, the real part of the conductivity

associated with interband transitions can be calculated analytically. For this reason,

using Eq. (2.20) when n = 1 in order to get the solution for the first order

conductivity, by substituting Eq. (2.41), Eq. (2.42), and Eq. (2.43) into Eq. (2.20), we

can calculate the first order optical conductivity of gapped graphene at T ≥ 0,

which can be derived as follows

∫ (

)

(

)

(

*

The second term is

(

)

(

)

The equations above can be reduced to the form of

(

*

(

*

(2.48)

where is the Heaviside step function. The total optical conductivity

of gapped graphene in the p-n junction regime will be determined from the sum of the

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57

intraband and interband transitions in the linear optical response by using Eq. (2.8)

and Eq. (2.48) for and in the THz regime as with Eq. (2.27).

In Fig. 2.6, we plot the frequency dependent linear optical conductance of a

graphene p-n junction with different band gaps. Here , and

the bias voltage at T =77 K. There exists a frequency region of 0-10

THz where the conductance is negative due to the interband transitions under the

condition As and , the conductance is twice the universal

conductance . In addition, increasing the gap size leads to a change in the

conductivity and a blue shift of threshold. Our results suggest that the linear optical

nonlinearity in both inter- and intra-band nonlinear optical processes can be enhanced

due to finite bandgap opening. nevertheless, the large gap opening leads to

degradation of the optical conductivity.The second order optical conductivity of

gapped graphene associated with interband transitions

is zero because of

time-reversal symmetry, which means that the total second order optical conductivity

will be zero.

Figure. 2.7 presents the change in frequency against the normalized real part of

the linear conductivity below for different temperatures of the Fermi-

Dirac distribution. Moreover, it can be shown that an increase in temperature leads to

a decrease in the negative linear conductivity of the gapped graphene p-n junction.

The value of the optical conductivity depends on the temperature, due to the

exponential increase in the number of electrons with temperature. Furthermore, as

temperature increases, the part of conduction band and valence band are thermally

occupied. This leads to reduce the carriers available for the optical transition and thus

reduces the optical conductivity. The behaviour of linear conductivity as a function of

temperature and band gap can reveal several interesting features such as a negative

conductivity in the limited range of THz frequencies, a blue shift of threshold

conductivity with the change in band gap at the Dirac point, and a reduction the peak

and width of the conductivity with increasing temperature.

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58

Figure ‎2.6. The real part of linear optical conductivity dependence on the frequency with

different band gap , where , and the bias voltage at

T=77 K.

Figure ‎2.7. Normalized real part of the linear conductivity vs. the frequency calculated for

different temperatures below with , and the bias

voltage .

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59

2.3.4 Nonlinear conductivity

The nonlinear optical response of single-layer gapped graphene under external

electric field has great importance for coherent terahertz radiation sources and

optoelectronic devices in the terahertz to infrared regime. It can play an important role

in developing graphene-based optical devices. Here, we are only interested in the real

part of the nonlinear optical conductivity due to interband transitions.

The nonlinear optical conductivity of the graphene p-n junction with the band gap

at the Dirac point that is associated with interband transitions can be determined by

modifying Equation (2.28) to make it appropriate for calculating the optical

conductivity of SLG below the band gap

(

)( )(

) (

)

Then, the equation above will be reduced completely to the form below

( )

(2.49)

and

∫ (

)

Where

( )

( )

so we have the third order optical conductivity at triple frequencies, as follows

[ ]

(2.50)

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60

The total optical conductivity is the sum of the intraband and interband linear

terms, the third order intraband nonlinear term, and the third order interband term. We

can calculate the frequency-dependent conductivity of gapped SLG in the p-n junction

regime as follows

(2.51)

We can solve Equation (2.51) by finding solutions to elements

and

by following the same steps that were used to solve the nonlinear optical

conductivity of gapless graphene, taking into account the energy gap.

[

( )

[ (

* (

*]

]

(2.52)

Where

(

*

(

*

(

) and

.

There are two third order nonlinear terms, and

. The interband

transition optical conductivity leads to a number of interesting nonlinear electronic

transitions. In Figure 2.7, it is shown that both the peak and width of the nonlinear

conductivity decrease as the band gap increases, while the linear conductivity peak

converges to zero. The band gap provides an additional mechanism for tuning the

position of the negative conductance peak.

Figure 2.8 shows the electric field intensity dependence of the nonlinear optical

conductivity below the gap. It is shown that the ratio of the nonlinear to linear optical

conductivity of gapped graphene increases with increasing frequency and electric

field.

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61

In Figure 2.9, the ratio of the nonlinear to the linear (intra- and inter)band optical

conductance of a gapped graphene p-n junction under moderate field as a function of

frequency in different electric field intensities and with , bias voltage

, and the band gap .

Finally, the nonlinear response in the gapped graphene p-n junction under

forward bias remains stronger in the terahertz regime than the linear response. The

negative optical conductivity of the p-n junction increases with increasing relaxation

time and gate voltage, and with decreasing temperature. The nonlinear response in the

gapped graphene p-n junction under forward bias becomes stronger in the THz regime

when a band gap is opened at the Dirac cone. Where, the nonlinear optical

conductivities exhibits two frequency optical response, i.e. there exists two distinct

absorption peaks in the optical spectrum. The absorption peak corresponds to three-

photon absorption is well separated from the linear response and this leads to the

existence of a frequency regime where the optical response is solely made up of the

nonlinear component.

Figure ‎2.8. The real part of the total linear and nonlinear optical conductivity of the

gapped graphene p-n junction as a function of frequency.

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62

Figure ‎2.9. The ratio of the real part of the nonlinear to the linear optical conductivity in

gapped graphene against the electric field intensity, with , bias voltage

, and the band gap .

Rat

io o

f N

onli

nea

r &

lin

ear

Op

t. c

ond

ctiv

ity

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63

2.4 Conclusion

In this Chapter, we studied the optical conductivity of the gapless and gapped

single layer graphene p-n junction in the terahertz regime under electric field with

intraband transitions by using the Boltzmann equation, and then we calculated the

linear and nonlinear optical response with and without gap that is associated with

interband transitions by adopt the quantum mechanical approach under a forward bias.

These results have an interesting consequence for the effect of the gap in the p-n

junction regime for the range of frequencies between 0-10 THz. Hence, bandgap

opening within limited size leads to an enhancement in the negative conductivity and

a blue shift of threshold. The band gap provides an additional mechanism for tuning

the position of the negative conductance peak.

It is worth noting the importance of the impact of bias voltage on the conductivity

in the terahertz regime of the graphene p-n junction, which leads to negative

conductivity when the bias voltage is greater than the photon frequency .

On the other hand, the negative conductance means that the electromagnetic field can

be amplified in this type of p-n junction.

The negative nonlinear optical response of the gapped graphene p-n junction

might be useful for device applications. The optical conductivity of the p-n junction

increases with increasing relaxation time and gate voltage, and with decreasing

temperature. The nonlinear response in the gapped graphene p-n junction under

forward bias remains strong in the terahertz regime. On the other hand, the

electromagnetic field can be amplified in this type of p-n junctions as a result to the

negative conductance. So, the relaxation time only affects the nonlinear processes

very weakly.

The oscillations of charges can lead to oscillations of the dipole momentum of the

system resulting, in the terahertz emissions [92]. In addition, using the gate voltage on

both sides of the p and n regions leads to control of the diffusion of electrons and

holes between the Fermi levels and can cause the junction to act as a processor to

convert potential oscillations into electromagnetic frequencies.

In the present study of the THz regime, the effect of electric field on the p-n

junction is also quite interesting. The ratio of the nonlinear to the linear optical

conductance in the gapped and gapless SLG increases with electric field intensity.

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64

With the same electric field intensity, the ratio decreases with increasing frequency.

When the electric field is weak, the nonlinear process is negligible. Also, the ratio

decreases with increasing frequency. The nonlinear conductance can be an order of

magnitude larger than the linear conductance when the electric field intensity is

around .

Finally, we found that the optical conductivity of the graphene p-n junction in the

THz regime with a gap is stronger than that without a gap. The nonlinear response is

more significant than the linear response due to the strong nonlinear effects.

These several interesting results can be useful for developing graphene based

optical devices and other optoelectronics device such as THz radiation sources

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65

Chapter 3

3 Strong Terahertz Photon Mixing in

Graphene

3.1 Introduction

Many interesting features of single layer graphene have been theoretically

predicted and experimentally observed, for example, electron-hole symmetry and the

half-integer quantum Hall effect, finite conductivity at zero charge-carrier

concentration, the strong suppression of weak localization, and the optical response in

the THz regime.

The optical and electronic properties of graphene are unique, and several of

them are still not understood, such as the unusually high carrier mobility [101, 102],

the absence of carrier backscattering [103], the existence of a universal optical

conductivity [26, 104], and a finite conductivity when the charge carrier density is

zero [105, 106, 107].

Strong terahertz interband [21] and intraband [22, 23] nonlinear optical

responses of single layer graphene have been predicted theoretically. In the visible

and infrared regime, a strong nonlinear optical response [24, 25] and frequency

multiplication of millimeter waves have been realized [108] This research lays the

foundation for using graphene in several valuable applications and devices at THz

frequency.

Under a moderate electric field of around , the nonlinear optical

response for gapless and gapped monolayer graphene has been calculated by using the

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66

quantum mechanical approach with the tight binding model in the THz to infrared

regime [21, 22, 97]. A strong nonlinear optical response for gapped graphene has

been observed in the THz regime. In addition, the terahertz nonlinear response of

bilayer graphene (BLG) has been calculated with the interband transitions, and it has

been shown that BLG can be the preferred material at room temperature and may

enhance the performance of optical devices [109].

Gap opening in monolayer graphene leads to improved and enhanced

optoelectronics devices and opens the door to fabrication of graphene based

devices, although they demand complex engineering [110, 111]. At low temperature,

the strong nonlinear optical response can be due to band-gap opening in semi-

hydrogenated graphene [112, 113]. This ferromagnetic semiconductor with a small

indirect gap had been previously studied by J. Zhou et al., who used the density

functional theory consider the removal of half of the hydrogen from a graphane sheet,

where graphane is a form of hydrogenated graphene [114].

The nonlinear response in the intermediate regime under finite temperature is

more important, as the practical implementation of a graphene-based device requires

finite temperature information, and also, finite doping is usually present due to crystal

imperfections and impurities. In this Chapter we study the photon mixing effect,

taking into consideration the full temperature spectrum of the nonlinear optical

response of a finite-doped ( ) graphene single layer in both the gapless and the

gapped cases, under both weak-field and strong-field conditions in the terahertz to

infrared regime.

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3.2 Photon mixing in single layer gapless graphene

In this section, we study and analyse the photon mixing effect in zero-gap

single-layer doped graphene at finite temperature and under weak field in the terahertz

regime, and then we consider the strong field case to calculate the linear and nonlinear

current over the full temperature range. We then calculate the critical electric field to

study the photon-mixing and strong interband nonlinear effects on the photon mixing

optical response of hot Dirac fermions. Figure 3.1 contains a schematic diagram of the

band structure of single layer gapless graphene and the photon mixing process of the

nonlinear optical response in both Dirac cones when and

Figure ‎3.1. Schematic diagram of the band structure of single layer gapless graphene and the

nonlinear photon mixing process when sign of the energy state .

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3.2.1 Formalism and theory

Firstly, we calculate the velocity operator and corresponding expectation value.

Around K or K' of the Brillouin zone, the Hamiltonian equation is a 2 × 2 matrix.

Under low energy conditions and in the tight-binding model of single-layer graphene

(SLG), the Hamiltonian can be written as

(3.1) |

|

Where the Fermi velocity is

, where is the

nearest neighbour hopping band width and is the C-C distance. The

energy eigenvalue of the 2 × 2 matrix of the Hamiltonian equation and of the

Schrödinger equation is obtained from the equation below,

(3.2)

| |

From Eq. (3.2), where are the positive and negative

energy states associated with the two symmetric branches, and at . The

velocity operator for Eq. 3.1, following Feynman [115], can be written as

(1.3)

( |

|*

We can write the expectation value of the velocity operator as ⟨ ⟩ .

From these equations, the velocity eigenvector can be expressed as

(3.4)

We consider a time-dependent applied electric field associated with strong

photon mixing in the THz regime in the form of

(3.5) ∑

Where , , and are the amplitude, wave vector, and frequency of the

wave of the electric field. Ignoring the weak magnetic component, the external

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field is minimally coupled to the quasiparticle by performing the substitution

, where and e is the electric charge. The velocity can

be expanded in the order of the electric field, assuming as

(3.6) (

| |*

Where

(3.7) ∑

[ ( )]

The linear and nonlinear velocities of the equation above (3.6) can be expanded

by using a Taylor expansion associated with the external field:

(

*

We can make some mathematical rearrangements in Equation (3.6). Thus, the

first, second, and third order velocity eigenvector can be expressed as

(3.8)

(

)

We can simplify the above equation as follows

(3.9)

(

*

(3.10)

(

)

(3.11)

(

)

(3.12)

(

(

*

(

*

(

*

)

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Equation (3.8) indicates that the zero-order velocity is equal to the Fermi

velocity when 1, which is consistent with the unperturbed case. In order to

obtain the current density, taking into account the Fermi-Dirac distribution, the

order current related to the velocity of gapless graphene is given by

(3.13)

∑∫ ∫

( )

Where

is the -order velocity of gapless single-layer graphene,

represents the chemical potential and is equal to the Fermi level, is the photon

energy, and and are the Boltzmann constant and the temperature, respectively.

is the thermal function of the Fermi-Dirac distribution, The integration above

can be solved by defining the limits of integration. At , the upper-limit cut-off,

is equal to the Fermi level and is arbitrarily set to a large value of for

and for numerical calculations. The value of the momentum

integration up to room temperature is well below , and hence, the choice of is well

justified. For , terminates the momentum integration at to avoid

the low-momentum regime where fails. Deep charge carriers cannot respond

to the external perturbation due to the unavailability of higher energy states. We

qualitatively approximate this by choosing a lower momentum integration limit

of .

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3.2.2 Linear optical response of gapless graphene

At zero temperature, we initially calculate the first order current when the

chemical potential μ is greater than the energy of the incoming photons by using Eq.

(3.11) and Eq. (3.9). Under the electric field, the linear current density can be written

as

∑∫ ∫

(

)

(3.14)

∑ ( ( ))

Note that there are two terms in Eq. (3.14). The first one is which refers

to the linear conductivity and is consistent with the linear conductivity calculated by

using the Kubo formula [105, 106], and the second one refers to the electric field for a

single incoming photon in single-layer gapless graphene at . The equation

above also agrees with the Drude formula at zero temperature. At , the current

density reverses direction and μ < 0. For , Equation (13.3) can be modified

under the thermal function distribution. This can be revised to a more reasonable

form, by defining

(3.15)

( [

]*∑ ( ( ))

The above Eq. (3.15) can be reduced to Eq. (3.14) when .

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3.2.3 Nonlinear optical response of gapless graphene

Now we calculate the second order current density, but due to the inversion

symmetry of graphene, the second order velocity

in Equation (10.3) does not

generate any electric current, so the second order current density is equal to zero. At

T , the third order current density can be written by using Equation (3.13) and the

third order velocity

in the terahertz regime. With applied electric field, we obtain

∑∫ ∫

(

3.16)

∑(

)

( [( )

( ) ])

The above equation is the same for the electron band when and the hole

band when at zero temperature due to the symmetry of the Dirac cones,

whereas represents the sum of the energy of three photons and

for and respectively. The third order nonlinear current

density for is given by

∑∫ ∫

(3.17)

∫ [

(

*]

( [(

) ( ) ]) .

In Eq. ( and Eq. ( , several interesting features can be observed. Firstly,

there is the impact of on the formula for the nonlinear current density of graphene

at finite temperature. A smaller generates a stronger nonlinear current. The

assumption of in the derivation of the nonlinear velocities is no longer valid,

however, if μ is too small, since this will involve charge carriers with momentum

comparable to .

Furthermore, the behavior of the temperature effects in relation to the third order

nonlinear current density is also quite interesting in the THz regime. Up to room

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temperature, the third-order nonlinear response is thermally enhanced, i.e., the third

order nonlinear current is enhanced with increased temperature. It should be taken

into consideration, however, that the nonlinear current does not grow to infinity with

increasing temperature. The charge carriers in the opposite Dirac cone contribute to

an opposite

generation at high temperature, which leads to a reduction in the

net nonlinear current. This reduction is not observed in our case because the , that

we have chosen is large. In addition, an increase in μ leads to an inversely

proportional decrease in the ratio of the nonlinear to the linear current density and

vice versa. Note that we used numerical calculations to solve Eq. (3.17) and used

analytical calculations for Eq. (3.16).

In Figure 3.2 we plot the dependence of the third order nonlinear current density

on temperature for three different (0.06, 0.08, and 0.10 eV) and .

We found that when the temperature decreases below approximately 150 K and

the chemical potential ( will have a negligible effect on the nonlinear

current density.

Figure 3.3 shows the temperature dependence of the third-order nonlinear current

density between and when for different (-0.06, -0.08, and -

0.10 eV), oscillating at . Our analysis indicates that the temperature and

affect the nonlinear current very strongly. In addition, when comparing Figure 3.2 and

Figure 3.3, we note that there is no symmetry between and in the third

order nonlinear current density of single-layer gapless graphene in the terahertz

regime, due to the asymmetry of the Fermi-Dirac distribution, while the temperature

dependence of the nonlinear current density is stronger than that of the linear current

density.

According to F. Gao et al., the 2-dimensional electron gas (2DEG) based Rashba

spin-orbit coupling exhibits a strong nonlinear response, which is of the same order of

magnitude as the linear current [116]. This is caused by the highly non-parabolic band

structure induced by Rashba spin-orbit interaction [117]. In our results for SLG, the

linear response causes smaller enhancement than that nonlinear response. The linear

response results in the same enhancement to the optical nonlinearity, however, and

this gives rise to the relatively stronger optical nonlinearity in comparison to F. Gao et

al. and P. A. Wolff [116, 117].

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Figure ‎3.2. Temperature dependence of the normalized third-order nonlinear current

density for at .

Figure ‎3.3. Temperature dependence of the normalized third-order nonlinear current

density for at .

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3.2.4 Critical electric field and Photon mixing effect

In this section, we evaluate the electric field effect of the contribution to the

photon mixing process in graphene that is obtained when 3 photons are included in

the nonlinear response calculation. In addition, to create a non-negligible photon-

mixing effect in graphene, the electric field can be determined by estimating | |

| | . Firstly, taking into account the electric field at by combining Eq.

(16.3) and Eq. (14.3), we arrive at the following equation:

∑ (

*

[( ) ( ) ]

∑ (

* [( ) ( ) ]

(3.18)

√ (

)

The above equation refers to the two incident beams and assumes that they have

the same intensity and polarization. In the terahertz regime ( ), the critical

electric field, Ec, in graphene is around V/cm at zero temperature with

. The critical field strength under these conditions is rather moderate and is

larger than the critical electric field of the nonlinear interband conductivity in single

layer graphene. Secondly, we can define a critical field at T > 0 by using Eq. (3.15)

and Eq. (3.17) when | | |

| , which is given as:

∫ *

(

)+

[( ) ( ) ]

( *

+)∑

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76

3.19

(

( *

+)

∫ *

(

)+

)

The above equation can be revised to a more reasonable form by making some

mathematical rearrangements to arrive at the following ,

where is the critical field and is a dimensionless parameter, which can be

expressed by

(

( *

+)

∫ *

(

)+

( )

)

Where

∫ *

(

)+

Therefore, the above equations can be used in rewriting as

3.20 (

( *

+)

| | |

|,

Equation (3.18) is related to the third order nonlinear optical response and the

temperature in graphene. Figure 3.4 indicates the change in temperature (

) against of the photon mixing regime for three different and .

Also, it allows a comparison between the critical field and the temperature. The

critical field at room temperature is about . Thus, at room-

temperature is approximately 10% lower than at T ≈ 150 K. This is consistent with

the experimental electric field strength where gigahertz waves mixing occurs [108].

In Figure 3.4, the scale for the x-axis runs from zero to room temperature, and

due to the linear response, increasing temperature leads to increasing at low

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77

temperature, but at high temperature, the nonlinear current rate overrides the linear

rate and leads to the peaking of . In addition, at room temperature, the critical field is

about lower than the critical field at , where the peaking of is

observable at when as shown in Fig. 3.4. Also, for

at room temperature, the is increased by approximately .

Figure ‎3.4. and the critical field Ec (inset) as functions of temperature in gapless graphene

for different when

We now estimate the electric field strength generated by the nonlinear

photon mixing of by using Maxwell's equation

(3.21) (

*

Where, is the d'Alembert operator. At distances far away from the quantum

well, the solution is approximately given by and the third

order polarizability is written as

(3.22)

(

*

(

*

60 120 180 240 300 T (K)

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3.2.5 Strong optical response photon-mixing in gapless

graphene under the strong field of hot Dirac Fermions

In this section, we calculate and discuss the optical response of carrier

population redistribution under the hot strong-field driven Dirac fermion regime

(SDF) in single-layer gapless graphene. In weak field, as in the previous part, the

Dirac-fermion distribution is described by where is the linear energy

spectrum. Under a strong field, that will not be longer valid, as the externally acquired

dynamics is

. In case of this dynamics, the Dirac-

fermion distribution will be quite different when and the

outcome will be different too, due to the inclusion of both distributions, with the Dirac

fermions acting to redistribute themselves. For the present system, the SDF can be

expanded as following

(3.23) ∑

where is the order derivative of , and it is necessary to calculate all

terms up to . This expansion can be used to rewrite equation (3.23) as

(3.24) (

*

(

)

(

)

Then, we proceed to calculate Equation (3.24), and neglecting all the terms over

n = 3, to arrive at the following equation

(3.25)

where

3.26

( (

)+

3.27

( (

) )

3.28 * (

(

*

(

*

(

*

)+

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where . To calculate the linear and non-linear current density equation

in the strong field regime, the above equations can be used in rewriting Equation

(3.13) as follows

3.29

∑∫ ∫

(

)

Firstly, we will calculate the first order term for the linear current density under

a strong field at zero temperature, by substituting Equations (3.26), (3.27), and (3.28)

into Eq. (3.29). It can then be shown that

(3.30)

where S and w refer to the weak and strong field cases. The equation above is

exactly equal to the first order current density under weak field when . Also,

when , the first order current under strong field is equal to the current for the

weak field. The second order current under strong field is equal to zero, as in previous

work. The additional second-order term vanishes after performing the angular

integration due to inversion symmetry.

(3.31)

At zero temperature, the third order current density under strong field ( )

can be written as

(3.32)

∑(

( )

)

[( ) ( ) ]

Equation (3.32) can be rewritten in a more reasonable form, by defining the left-

hand side in the following way:

(3.33)

Where

(3.34)

(

*∑

( [( ) ( ) ])

where S and refer to the optical responses of the strong (SDF) and weak field

Dirac-fermion (WDF) cases, respectively. In addition, for Equations (3.30) and (3.31),

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it is worth noting and interesting that whether under weak or strong field, the first and

second-order nonlinear optical responses of graphene are not changed, although the

whole SDF population has redistributed itself. This refers to the population

redistribution phenomenon induced by the strong field. In other words, the linear

current density is protected from the strong field effect.

At and under a strong field, the third order current density can be

expressed by rearranging Eq. (3.33), so that the first term

is as calculated

previously (see Eq. (3.17)) and the strong field term

is given as

(

( *

)

( [(

) ( ) ])

The above equation will then be reduced to the form of the equation below

(3.35) (

)

(

( *

)

Finally, the total third order current density under SDF and at is defined

as

(3.36)

Eq. (3.36) is an expression of the strong nonlinear optical response of gapless

single layer graphene under strong field (S) and is a description of how strongly the

Dirac fermions respond in the SDF case to an external perturbation. The degree of

redistribution depends on the coupling between the externally acquired dynamics and

the unperturbed dynamics of Dirac fermions in the WDF case at T ≥ 0.

In the previous section, the critical electric field at zero temperature was

calculated by using the estimate of the electric field intensity such that | |

| | , but now we are going to calculate the strong critical electric field at

, which is given as

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(3.37)

[

]

From the above equation, we can observe that is smaller than

by approximately three times, and when and the strong critical

electric field is approximately equal to 3300 V/cm, as shown in Figure 3.5. Secondly,

in this section, at finite temperature the strong critical electric field for SDF can be

derived as

(3.38)

(

( *

+)

∑∫

(

( )

,

)

The equation above can be determined by using the dimensionless parameter β

and comparing between the strong critical field at and such that

, so one can write

(3.39) (

( *

+)

,

The behaviour of is also quite interesting, because it describes the strong

nonlinear optical response under strong field as a function of temperature. Figure 3.5

shows the temperature dependence of the strong critical electric field oscillating at

in comparison with the weak critical field for WDF. The temperature

dependence of the dimensionless parameter is shown with three different . Also,

the Figure shows that is lower than

and there is a wide temperature range from

to . Under strong field, the

leads to amplification of the

third order nonlinear optical response in graphene under hot Dirac fermions.

Therefore, in Figure 3.5 we can observe the strong third order nonlinearity in SDF in

comparison to the normal Dirac-fermion WDF.

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The hot Dirac fermions play an important role in the optical response in

graphene due to the non-equilibrium nature of these hot Dirac fermions in graphene.

The hot Dirac fermions in graphene are short lived, especially in the case of a high

lattice temperature, where stronger electron–phonon coupling provides an efficient

pathway for relaxation [118] So, the electron temperature, for the hot electrons is

higher than the lattice temperature in the SDF regime [119]. In WDF, the hot-

electron becomes equal to . On the other hand, in the strong-field regime,

the non-equilibrium heating of SDFs lifts the SDF temperature above the lattice

temperature, and hence, the temperature terms in Eqs. (3.30), (3.33), and (3.36) must

be replaced by , where is the hot electron SDF temperature and > .

Figure 3.6 contains the temperature dependence ratio of the third order

nonlinear current density at finite temperature ( to that at zero temperature

under the SDF regime at three different chemical potentials. It shows that for the hot

temperatures between to , the nonlinear optical response

in the SDF regime is stronger than in the case of equilibrium Dirac fermions where

. Note that the lattice temperature is up to [120].

Finally, in the photon mixing process and the optical response of single layer

gapless graphene under the strong field with hot Dirac-fermions, several interesting

features can be observed. The first and second order optical responses are unchanged

by the high field because of the Dirac fermion dynamics and the inversion symmetry

of the graphene structure. Furthermore, the third order nonlinear optical conductivity

is intrinsically proportional to and can be enhanced due to the externally acquired

dynamics

by the strong-field-induced carrier population redistribution. The

nonlinear current density is enhanced by the non- equilibrium hot Dirac fermions

when is greater than which leads to a rise in the electron temperature.

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Figure ‎3.5. Temperature dependence of the critical electric field at and

for different critical field cases: (i) weak field (ii) strong critical field

both under SDF. The inset shows the temperature dependence of in the strong field of hot

Dirac fermions.

Figure ‎3.6. Temperature dependence of the third order nonlinear current density at finite

temperature ( normalised by that at in the SDF regime with three different

chemical potentials.

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84

3.3 Photon mixing in single-layer gapped graphene

The linear and nonlinear optical effects in gapped graphene are discussed in this

section. Pure graphene is a semiconductor without an energy gap, where the upper

band and the lower band meet at the Dirac point, giving it many exciting electronic

properties. Many electronic applications cannot be achieved, however, because there

is no gap at the Dirac point to control the properties of the semiconductor. A zero-gap

graphene-based transistor cannot be switched „off‟, and this causes a technical

problem for electronic equipment. Recently, there have been many experimental and

theoretical reports on tuning the band gap to realize a finite gap in graphene [111-113,

65, 121]. In addition, many methods have been used to open and tune the band gap,

such as the heteroatom doping and chemical modification methods, as well as using

an electrostatic field to tune and control the Fermi level [65, 66, 122, 123]. Also,

stacking graphene in a suitable way can also result in band-gap opening due to

sublattice symmetry breaking [99].

A nonlinear optical response in zero-gap graphene can be achieved in single

layers and bilayers by applying moderate electric field around [21,

22, 97], and the nonlinear current of gapless graphene increases with increasing

temperature in the important terahertz frequency regime. On the other hand, up to

room temperature, this nonlinear effect is thermally enhanced [124, 125].

Furthermore, the optical nonlinear response can be optimized as a result of the Dirac

behaviour of the graphene quasiparticles due to the low Fermi level and electron

filling [125, 126].

In the present section, we calculate and analyse the nonlinear photon mixing

effect of finite-doped gapped single-layer graphene under weak field and strong field

in the terahertz regime. Then, we adopt the strong field of the hot Dirac fermion

distribution to study the effects of a band gap on the photon mixing process,

compared to the case of gapless graphene in the terahertz frequency regime. Then, we

use the dimensionless parameter β to describe the temperature dependence of the

optical nonlinear and linear behaviour at low and high temperature.

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85

3.3.1 Formalism and theory

To calculate the nonlinear current density in gapped single-layer graphene, we

take into account the Hamiltonian equation with the band gap in the low energy

regime near the Dirac point in the tight–binding equation. The Hamiltonian of a

massive Dirac fermion for this system can be written as follows

.

(3.40) |

|

where is the finite energy gap in the different sub-lattices. The energy

eigenvalue can be obtained by substitution of Eq. (3.40) into Eq. (3.2), and is given by

2.

(3.41) √

The equation of the energy eigenvalue indicates band gap opening of at the

K-Dirac point. The velocity operator for Eq. (3.40) can be written as

3.

(3.42)

( |

|*

The expectation value of the velocity operator is given by ⟨ ⟩ . The

velocity eigenvector can be written as

The velocity can be expanded in the order of the electric field, assuming .

It can be derived as follows

(2.3)

By using similar procedures to those for gapless graphene, the linear and

nonlinear velocities of the equation above (3.43) can be expanded by using a Taylor

expansion on the external field, which is given by

(

*

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From Eq. (3.43), the total linear and nonlinear velocity eigenvector up to third

order in the external field can be expressed as follows

(3.44)

√( )

(

( )

( )

( )

( )

( )

( )

(

)

( )

+

We can rewrite the above equation in a more reasonable form as below

(3.45)

(3.46)

√( )

(

( )

)

(3.47)

( )

(

( )

)

(3.48)

( )

(

( )

( )

( )

+

Now, we proceed to calculate the current density in the order current related

to the velocity of electrons in gapless graphene with the Fermi-Dirac distribution,

which is given by the previous current equation (3.13). We also calculate

in the

-order velocity of gapped graphene up to third order.

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3.3.2 Linear optical response of gapped graphene

In this section, the first order velocity is used to obtain the linear current density

in zero temperature of gapped graphene

by substituting Equation (3.46) into

Eq. (3.13). It can be shown that

( )

( )

∫ ∫

( )

( )

where is the angle between and u, and . The equation

above can be solved analytically at zero temperature and can be written as

(3.49)

[

( )

(( ) )

]

Now, we are going to rewrite the linear current equation in dimensionless form,

which allows comparison between gapless and gapped graphene at zero temperature

where

, leading to the equation below

(3.50)

[

(

*

(

*

]

The dimensionless parameter represents the effect of gapped on the linear

current density at zero temperature. Now, Eq. (3.50) can be used to rewrite Eq. (3.49)

as

(3.51)

For , the first order linear current under the Dirac-Fermion thermal

function can be determined by

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∑∫ ∫

( )

(

)

(

)

(3.52)

( (

))

Equation (3.50) can be solved numerically for , and the term

refers to the linear conductivity.

3.3.3 Nonlinear optical response of gapped graphene

To calculate the second order current density of gapped graphene, we use the

second order velocity

and substitute it into Equation (3.13). The result is found

to be equal to zero as a result of the inversion symmetry of the graphene crystal. We

now calculate the third order nonlinear current at zero temperature by substituting the

third order velocity

in Eq. (3.47) into Eq. (3.13), and the result can be

expressed by

(3.53)

∑(

)

where [( ) ( ) ]. The equation above can be solved

analytically by changing the Fermi-Dirac distribution to a step function. We can also

write the above equation in a more suitable form in order to compare gapless and

gapped graphene at zero temperature, by using a dimensionless parameter such that

. It can be shown that

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(3.54)

( (

*

)

( (

)

)

( ( )

)

( ( )

)

The dimensionless parameter represents the effect of the half-gap on the

third order nonlinear current density at zero temperature. Eq. (3.53) will then be

reduced to the form of

(3.55)

(

*

At finite temperature, the nonlinear current of gapped graphene under the

Fermi-Dirac thermal function can be written by modifying Eq. (3.13) and using the

third order velocity for the case with the band gap, as follows

( )

(

( )

( )

)

(3.56)

∑ ∫ (

(

)

( )

,

(

)

Where

( [( ) ( ) ])

For the nonlinear optical response is solved numerically and is cut off at

the upper limit of .

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3.3.4 Critical electric field and Photo mixing effect

In the present case, we have adopted the assumption of proportionality between

the linear and nonlinear current density to calculate the critical electric field strength

in gapped graphene as | | |

| . Now, we calculate the critical field at zero

temperature from the proportionality equation, as

(3.57)

(

(

)+

At finite temperature, the critical electric field strength can be found by using

the proportionality between Eq. (3.52) and Eq. (3.56), and using similar procedures to

obtain | | |

| . The dimensionless parameter at finite

temperature is defined as

, where

(3.58)

(

| | |

|∫

( (

)))

On the other hand, the critical field strength for gapped graphene is also given

as , where is the zero temperature critical field strength of gapless

graphene and √ . The dimensionless factor indicates the effect of the

band gap on the critical field strength.

In Figure 3.7 we plot the dimensionless factor as a function of the band gap,

which changes for different chemical potential at at zero temperature. At

and , when and at zero temperature, the

linear optical response in gapped graphene can be enhanced by the factors

and . In addition, the nonlinear optical response will be enhanced by

the factors and . This leads to a reduction of the critical field by

the dimensionless factor and . This means that the

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nonlinear optical response in gapped graphene is improved by approximately 8%

compared to the nonlinear optical response in gapless graphene. In addition, where the

band gap is large, will be greater than one, and thus the nonlinear optical response

will be degraded because many low lying states will be destroyed. At high

temperatures, the enhancement of the optical nonlinear response will not continue in

this regime. Therefore, we suggest that the optical nonlinearity enhancement due to

band-gap opening is universal to both inter- and intraband nonlinear optical processes.

So, we suggest keeping less than one to enhance the nonlinear optical response by

controlling the band-gap size.

Figure ‎3.7. Band-gap dependence of with three different at zero temperature and

.

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3.3.5 Strong optical response photon-mixing in gapped

graphene under the strong field of hot Dirac Fermions

We proceed to calculate the optical response under the strong field of hot Dirac

fermions. In the previous part, the Dirac-fermion distribution is described by the term

( ) where ( )

is the unperturbed gapped single-layer

graphene linear energy spectrum under weak field. This is no longer negligible under

strong-field conditions, however, and thus the externally acquired dynamics will be

taken into account by assuming the hot Dirac-fermion distribution function and

( ) where represents the carrier energy under

strong field and (

) . We then use a similar procedure

as for gapless graphene and expand up to the third order velocity, where (

)

indicates that the carrier population redistributes

itself. Under the SDF regime, we will expand Eq. (3.23) to arrive at the following

equation

( ) (

) (

)

(

)

(

)

(

) (

)

(

)

We take into consideration the velocity up to third order, where is the thermal

Dirac-Fermi distribution function. We can rewrite the above equation in simple and

uncomplicated form as

(3.59) (

)

(3.60)

(

)

(

)

(3.61)

(

) (

) (

)

(

)

where

and

is the expectation of the velocity in gapped

graphene from Equations (3.44), (3.45), and (3.46) up to n = 3. The linear current

density at zero temperature in gapped graphene under strong field can be obtained by

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(3.62)

∑ ( )

(3.63)

(3.64)

The equations above can be solved analytically. They show that both the linear

and the nonlinear optical responses in gapped graphene are affected by the strong

field SDF, in contrast to the linear optical response in gapless graphene. The second

order optical response still remains zero in the strong field regime, however.

For , the linear and nonlinear current density is numerically calculated

under the thermal function distribution. This can be rewritten in more reasonable

form, by defining

(3.65)

∑ ∫

(

(

) +

where

(

*

(3.66)

where

represents the additional field term under strong field. We

evaluate the electric field strength under the SDF regime by using a similar procedure

to that for gapless graphene and estimate the value of the ratio of the nonlinear

current of gapped graphene to the linear current density at zero temperature such that

1. We can then write the electric field strength equation under the

SDF as

(3.67)

( (

(

)

))

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3.4 Conclusion

We have studied and calculated the linear and nonlinear current density of

single-layer gapped and gapless graphene and it‟s temperature dependence (zero

temperature and finite temperature) in both weak field and strong field of the Dirac-

fermion distribution. Firstly, in gapless graphene, it was demonstrated that the

nonlinear current effect increases with temperature up to room temperature, and is

very much stronger than the linear current density. So, the nonlinear effect is

approximately inversely proportional to the Fermi level. The third order nonlinear

optical response is asymmetric between due to the finite

temperature Dirac-fermion distribution of electrons and holes in graphene based

material. In addition, asymmetry is created by the strength of the electric field effect

when it is around .

Under the strong field of hot Dirac fermions, the optical response exhibits

strongly nonlinear behaviour, and the nonlinear optical response of SDF is stronger

than for the equilibrium Dirac fermions where the lattice temperature is equal to or

lower than room temperature. Furthermore, the first and second order optical response

is unchanged by the high field of SDF, and the third order nonlinear response can be

stronger than that in weak field because of the externally acquired dynamics, leading

to a redistribution of the carrier population.

Secondly, in gapped graphene, we found that the nonlinear optical response in

gapped graphene is enhanced by approximately 8% over the nonlinear optical

response in gapless graphene under weak field at zero temperature and finite

temperature, and it increases with increasing temperature with a finite gap. For a large

gap, however, the nonlinear optical response will be degraded due to the destruction

of many low lying states. At high temperatures, the enhancement of the optical

nonlinear response will not continue in this regime.

Under strong field SDF, the Dirac-Fermion distribution will be different from

that with the weak field as ( ), and this leads to the

stronger nonlinear optical response under SDF than that under WDF. On the other

hand, it shows that both the linear and the nonlinear optical responses in gapped

graphene are affected by the strong field SDF in comparison with the linear gapless

graphene. The second order response is equal to zero in both the strong field and the

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weak field regimes of gapped and gapless graphene due to the inversion symmetry of

the graphene structure.

In view of the fact that the strong nonlinear optical response in gapped or

gapless graphene can be enhanced by temperature and under strong field SDF,

graphene is a perfect material for many applications related to graphene based sources

in the terahertz regime and might be utilized in optoelectronic devices in modern

electronics.

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Chapter 4

4 Nonlinear Optical Properties of

Bilayer Graphene in the Terahertz

Regime

4.1 Introduction

Over the past few years, since the fabrication of monolayer graphene (MLG),

MLG has predominated in many recent research reports, such as on the quantum Hall

effect, finite conductivity, and the strong nonlinear optical response in the terahertz

regime. Recently, bilayer graphene has been reported in many interesting

experimental and theoretical reports [127-131], as it provides new and different

electronic properties that are not seen in single layer graphene, for example, the

triangle warping around the K point at zero energy [86, 132], the quantum Hall

effect, and a tunable band gap, while the electrons in bilayer graphene (BLG) also

show different behaviour than in the monolayer.

The band gap in the electronic band structure of BLG, which is tuneable by a

gate voltage, has been studied theoretically by Hongki et al. [81] by using ab initio

density functional theory, as well as by using the tight-binding model to control the

gap [85, 133-137] and describe the optical properties, along with the integer quantum

Hall effect [138] and the energy dispersion of BLG or few-layer graphene near the

Dirac point, which can be tuned by a gate voltage or doping [139,140]. The quantum

Hall plateaus in BLG are doubled and are independent of interlayer coupling strength.

On the other hand, the electron transitions between the two layers have shown the

important influence of the interlayer coupling parameter on the optical absorption,

in contrast to monolayer graphene and independent quasiparticle [141, 87].

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The lattice structure of bilayer graphene (honeycomb crystal structure) can be

found in two configurations of the honeycomb crystal structure: (i) the two layers in

the bilayer are symmetrical, where unit A1 in the top graphene sheet lies above unit

A2 in the bottom graphene layer, and B1 above B2 in a similar way; or (ii) the two

sheets in the BLG are asymmetrically stacked, where unit A1 in the top graphene

sheet lies directly above unit B1 in the bottom graphene sheet, which is called Bernal

stacking, as shown in Figure 4.1(a). The atomic structure in such bilayer graphene

with three hopping parameters is shown in Figure 4.1(b), where is the hopping

parameter between nearest-neighbour sites in each layer. represents the hopping

between A1 and B2. Finally, is the hopping parameter between B1 and A2 [136,

79]. This asymmetrical arrangement is the most common, and this asymmetrical

stacking can lead to a gap between the conduction band and the valence band [142,

129]. Opening the gap in BLG will open the way for graphene to become a candidate

for many optical and electronic devices in Nano-scale applications. One of the most

remarkable properties of the optical terahertz response can be enhanced in the

nonlinear regime of BLG. This optical response was also studied by using many-body

Green's function theory [143].

In Chapters 2 and 3, we studied the linear and nonlinear optical properties in

single layer graphene, and we adopted the quantum mechanical approach to calculate

the linear and nonlinear current and conductivity. In this chapter, we will shed light on

the linear and nonlinear optical response of bilayer graphene in the terahertz to

infrared frequency regime. Under moderate electric field intensity and by using an

approach that treats the coupling of Dirac electrons to the time dependent electric

field quantum mechanically, we calculate the strong nonlinear term for the case of

multiple photons. We also determine the required field strength to induce non-

negligible nonlinear effects.

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Figure ‎4.1. (a) Schematic diagram of the atomic structure of bilayer graphene. Solid lines

indicate the top layer, and dashed lines indicate the bottom layer. (b) Schematic diagram of

the atomic structure in bilayer graphene with three hopping parameters. is the hopping

parameter between nearest-neighbour sites within each layer. represents the hopping

between A1 and B2, and between B1 and A2.

𝜸𝟏 𝜸𝟎

𝜸𝟑

𝜸𝟎

A1

A1,B2

A2

A2

B1

A1,B2

A2

A2

B1

B1 B1

B1 B1

A1,B2

A1,B2 A1,B2

A1,B2

B1

a

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4.2 Formalism and theory of Hamiltonian in bilayer

graphene under the low-energy

To model the bilayer graphene as two coupled hexagonal lattices including

in-equivalent sites A, B and , in the bottom and top layers, and takes into

account the trigonal warping, we use the gapless Hamiltonian equation around K-

point and which is described by a 4 ×4 matrix. Tight-binding Hamiltonian in the basis

in the K and in the basis in the can be written as

(

,

Above equation can be simplified if one assumes . By eliminating high

energy states and reduce the previous 4 × 4 to a 2 × 2 Hamiltonian which describes

the effective interaction between the non-dimer sites A1-B2. In this section, we can

write a two-band effective Hamiltonian describing low-energy states to evaluate the

topological properties of this effective Hamiltonian. So, we determine the

Hamiltonian equation for gapless bilayer graphene by using the tight-binding

approximation in near energy minima under a time-dependent applied electric

field , whose direction is along the x-axis, under the effective mass

approximation, which can be written as[20, 21, 24]

(

) (

+ (4.1)

where , , . is

with reference to the K point (Dirac point), and . We can rewrite

Equation (1.4) in a more suitable form as

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(

)

(4.2)

The wave function for BLG can be written as in the equation below

and the term can be expanded into two spinor components, and

in the order, as follows

∑(

*

(4.3)

Now, we calculate the two spinor components in the order. By substituting

Eq. (4.2) and Eq. (4.3) into the Schrödinger equation , we obtain:

Left hand side of the equation

(

* (4.4)

Right hand side of the equation

(

(

)

(

)

)

(4.5)

Then, we can revise Eq. (4.4) and Eq. (4.5) into a more suitable form in the

order by defining

(

) (

* (

*

(

*

(4.6)

Now we can solve Eq. (4.6) and absorb the and into the spinor

components to obtain , and , respectively. Therefore, this

equation can be expressed as

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(4.7)

and

(4.8)

where ( ), and . When the electric field

is greater than zero, the terms and are non-zero, however,

when the electric field equal to zero, only n = 0 terms are non-zero. Generally, the

normalization and solution of Eq. (4.7) and Eq. (4.8) of wave function in zero order

can be defined as

(

)

√ (

, (4.9)

where is the eigenvalue in zero applied field. From the Hamiltonian equation,

the energy dispersion is found to be

(

) (

*

where υ is the angle between the energy distribution and the momentum of the

graphene band structure, and the sign ± represents the two sides of the energy bands

of BLG. The energy dispersion equation has four solutions describing the four energy

bands, as shown in Figure 4.2. Two of them do not touch the K point and relate to the

interlayer coupling, while the other two touch K points and describe the low energy

bands for gapless graphene (the absence of layer asymmetry [87]). The equations

above can be reduced to the form of

√ (4.10)

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Figure ‎4.2. Schematic diagram of the four low energy bands around K points.

The eigenvalue equation gives descriptions for all the photon processes in pure

gapless bilayer graphene. The term solution of Eq. (4.7) and Eq. (4.8) can be

calculated up to n = 3, as follows

The first order solution of when

√ (

)

(4.11)

Likewise, for the solution of we obtain

√ [

]

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√ [ ] (4.12)

The second order solution of can be obtained as follows

√ [ { }

[

] ]

(4.13)

[ ]

[ ]

(4.14)

Finally, the third order solution of when can be obtained as

[ ]

(4.15)

And

(4.16)

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4.3 Current density formalism and theory

In this section, the current density of gapless bilayer graphene will be

determined by using the current operator and the velocity operator in the terahertz to

infrared regime under applied field and at finite temperature. The order current

density can be calculated from the equation below

(4.17)

where is the thermal factor and is given by the Fermi–Dirac function

distribution as

(

)

(( )

)

(

*

(4.18)

The result is the equivalent finite temperature, where is the current operator,

which is expressed in the following terms:

(4.19)

here represents the proportionality of the current density to the power of

the electric field. It can be defined in terms of the linear and nonlinear

proportionalities as follows

*

+

*

+

(4.20)

The total current density is the sum of the first order linear current density and

the third order current density. In addition, we can calculate the optical conductivity

of bilayer graphene through the general equation for the current, which involves the

influence of an electric field, as follows

( ∑

+

The linear and nonlinear optical conductivity for bilayer graphene can be

calculated by using Eq. (4.20).

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4.3.1 Velocity operator formalism in the current density

equation

The velocity operator from the Hamiltonian matrix is obtained from the

equation below

(

) (

*

(

* (

)

(

) (4.21)

he equation above is the velocity operator along the x-axis and is split into a

quadratic part and a linear part . If 0, the vector will contribute

to the current density equation, and will be absent from the interaction. In

addition, the velocity direction along the y-axis is given by

(

) (

*

(

( )

( ) ) (

)

Also, the equation above is split into a quadratic part and an imaginary

linear part . It can be rewritten as follows

(

( )

( ) ) (4.22)

In this chapter, we will assume that the real part of the velocity operator lies along the

x-axis.

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4.4 Linear optical response of bilayer gapless graphene

In this section, we will proceed to calculate the first order linear current density

in the terahertz regime in gapless BLG at finite temperature. By substituting the first

order linear part of Eq. (4.20) into of Eq. (4.17), we obtain

where is the first order current operator and can be considered as the follows

*

+

Then

[∫

] (

* (4.23)

[∫

(

* (

)

(

* (

)] (

*

The equation above is complicated, so we will divide the equation into two terms

to solve it easily as follows

∫[

( ) ( ) ] (

* (4.24)

∫[

( ) ( ) ] (

* (4.25)

By substituting Equations (4.9), (4.11), and (4.12) into Eq. (4.24), we obtain

(

)

To solve the above equation, it is more suitable to convert the integration as

follows

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(

*

where is the analytic factor of the denominators; therefore the Dirac function

can be defined by the analytic continuation of the denominators as

(

*

(4.26)

where

( )

|

By using the cosine rule, where , we can derive the following

results from the above equation

(4.27)

(4.28)

|

|

√ (4.29)

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Finally, we will obtain the first order linear current density as follows

(

)

(√

) (

* (4.30)

The equation above can be solved numerically. By using the same method as for

Eq. (4.25), we can find the solution to Equation (4.30). Thus, the total first order

linear current is given by

(√

) (

*

∫ (

*

+) (

)

(4.31)

where √

. The result for the first order

linear current density is equivalent to the linear result from the Kubo formula. The

integration limits (upper and lower) can be calculated in order to avoid the infinite

parts by cutting off the integration limits at the known upper and lower limits, as in

the following calculations to find the upper K and lower K integration limits, by

using Eq. (4.27) and Eq. (4.28)

where

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After solve this equation we get four solutions for k

( √

+

( √

+

( √

+

( √

+

(4.32)

Finally, we will substitute the equation above into Eq. (4.31) to find the

numerical solution for the first order current density and find the linear optical

conductivity for bilayer graphene.

4.5 Non-linear optical response of bilayer gapless

graphene

The second order solution makes no contribution due to time-reversal symmetry.

Therefore, we will proceed to solve for the third order current through the use of the

general current equation as mentioned in the discussion for the first order, and we

also can calculate the third order conductivity. So, the general current equation can be

written as follow.

∫(

)

(4.33)

We can expand and simplify Eq. (4.33) by defining variables and substituting in

the values of variables, according to the above-mentioned equations. The result can be

obtained as the form below

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(

( )

( ) ) (

)

( ( )

( ) )(

)

( ( )

( ) ) (

)

( ( )

( ) )(

)

and then

( ( ) ) ∫ ( ( ) )

∫ ( ( ) ) ∫

( ( ) )

∫ ( ( ) ) ∫

( ( ) )

∫ ( ( ) ) ∫

( ( ) )

There are two distinct third order currents: One oscillates with , and the

other oscillates with , , where the combination of , , , and

contributes to ; and the combination of , , , and contributes to

.

So, we can rewrite the above equation in two forms to make it easier to solve more

accurately, as in the equations below

∫( ( ( ) )

( ( ) ) ) (4.34)

∫( ( ( ) )

( ( ) ) ) (4.35)

Here, we will divide the above integrals into two parts to avoid an error, as

follows,

First Equation (4.34),

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∫ ( ) ∫

[

{

[ ]} {

[ ]} { [

] [ ]}]

∫ ( ) ∫

{

[ ]

[

]}

Second Equation (4.35)

∫ ( ) ∫

[

[

{ }]

[ {

}]

[{ } {

}] [ { }

{ }]]

∫ ( ) ∫

[ (

)] [

{

}] { [ ]

[ ]} {

}⟩

The above equations are solved by using numerical methods. The method to

solve the third order current and non-linear conductivity within the limits of

integration mentioned previously in Equation (4.32) has been used to obtain the

solutions.

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4.6 Results and discussion

T This chapter is focused on calculation and analysis of the linear and nonlinear

optical conductivity in bilayer graphene, by using the low-energy Hamiltonian

equation for gapless bilayer graphene and by using the tight-binding approximation

under electric field. There is a particular focus on the important frequency regime of

the terahertz to far-infrared.

In the first section we calculated the linear conductivity in this frequency range as

shown in Figure (4.3). In this Figure we plot the linear conductivity versus frequency

in units of

the universal conductance. Also, the total current in Equation

(4.31) with n = 1 terms is equivalent to the linear response result obtained from the

Kubo formula. On converting the conductivity into real units, the linear conductance

result at low energy is equal to when . Furthermore, the second order

solution of the current density makes no contribution and is equal to zero due to time

reversal symmetry.

In the second section, we calculate the real part of the nonlinear optical

conductivity for the n =3 term in units of . We used the numerical result to plot the

third nonlinear optical response against the frequency for different temperatures (0-

300 K) and under electric field (see Figure 4.4). This figure shows that

the nonlinear optical conductivity decreases gradually with increasing frequency.

Also, it shows the effects of temperature on the optical conductivity as expressed in

two third order conductivities, One oscillates with the frequency , and the

other oscillates with , .

In Figure 4.5, we plot the normalized nonlinear conductivity in units of

versus temperature at a field of 600 V/cm and 1 THz frequency. From this figure, it

can be observed that the nonlinear conductance of exceeds the linear

conductance at low temperature, while the is smaller than the linear term at low

temperature. The is greater than the linear conductivity at most temperatures,

however. As a result, we can say that the all important stays about the same as

the linear conductance at room temperature. This result suggests that bilayer graphene

could be a candidate for the development of optical instruments and nonlinear

terahertz photonic devices.

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The third section presents the effects of the electric field on the optical response

and also describes the critical electric field, which leads to the equality between the

linear and nonlinear optical response at a specific field, which represents an important

feature of the nonlinear response, as shown in Figure 4.6, which displays the critical

fields at zero and room temperature as a function of the frequency within the range of

0-5 THz, where the electric field is well within that range due to the field strength

achievable in the laboratory. In addition, we can observe two critical fields,

and and the critical field increases with increasing frequency and

temperature, as shown in Fig, 4.6, This result is similar to the nonlinear effect for a

single layer. This result suggests that interlayer coupling and doubling the carrier

numbers in BLG do not reduce the nonlinear effect [109].

On the same subject, Fig. 4.7 shows the relationship between temperature and the

critical electric field. It also shows the rapid decline of the critical field at low

temperature as a result of the decrease in the linear current, while increasing the

temperature over leads to stability of the electric field, which is primarily due

to the thermal occupation of the bottom and top part of the conduction band and

valence band, respectively. This consequently leads to a reduction in the available

carriers and the mechanism behind optical transitions, leading to a decrease in the

linear current.

Finally, bilayer graphene has strong nonlinearity, more than other such materials.

This nonlinear effect is robust from low to room temperature. Also, the nonlinear

optical response is stronger than the linear response. BLG exhibits a strong nonlinear

low energy response due to the unique properties of BLG, especially the warping

trigonal property.

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Figure ‎4.3. Linear optical conductance as a function of frequency at zero temperature.

Figure ‎4.4. Nonlinear optical conductance as a function of frequency at zero and room

temperature, with the electric field set at 1000 V/cm.

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Figure ‎4.5. Normalized nonlinear conductivity in units of versus temperature at field of

600 V/cm and 1 THz frequency.

Figure ‎4.6. Critical electric fields at zero and room temperature as a function of the frequency

within the range of 0-5 THz.

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Figure ‎4.7. Critical field vs. temperature at frequency of 1 THz.

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4.7 Conclusion

In this chapter, we summarize some of the features that can be identified from a

study of the optical response of gapless bilayer graphene. We have also achieved a

suitable theoretical approach to calculating the linear and nonlinear current density by

using the tight-binding approximation near energy minima and in the terahertz to far-

infrared regime through the Schrödinger time-dependent equation including applied

electric field. In addition, we expanded the Schrödinger equation to confirm the four

energy bands for bilayer graphene, in which two of them do not touch the K point and

are related to the interlayer coupling, while the other two touch K points. They thus

provide a description of the low energy bands for gapless graphene (in the absence of

layer asymmetry).

To analyze our results, we take into account models for the optical response of

graphene bilayer based on the electronic system described by the Fermi-Dirac

distribution at different temperatures and in the important frequency regime. In this

chapter, several interesting features can be observed. One of the main features is that

the first order linear optical conductivity is equal to when , and the second

order is equal to zero due to time reversal symmetry. Secondly, the nonlinear effect is

strong for a wide range of temperatures within a specific area that extends from low to

room temperature. Thirdly, there are single frequency and frequency tripling

nonlinear terms, the latter of which is comparable to the linear term in the terahertz

frequency regime and under very moderate electric field. The field strength for the

nonlinear effect in bilayer graphene is well within the experimentally achievable

range in laboratories. In addition, bilayers may be preferred structures for developing

graphene-based nonlinear photonic and optoelectronic devices.

We have also noted the effects of temperature on the optical conductivity.

Increasing the temperature from low to room temperature leads to a decrease in the

optical conductivity for electric field of . Furthermore, the linear

conductance at low temperature has less impact than the nonlinear conductance of

, while at low temperature, the frequency tripled nonlinear response becomes

smaller than the linear term within the same frequency range.

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On the other hand, the behavior of the nonlinear current density and conductivity

in different frequency ranges is also quite interesting. The nonlinear optical response

decreases gradually as a result of an increase in the frequency. Also, the single

frequency nonlinear response is greater than the frequency tripled nonlinear response

in different frequency ranges.

It is worth noting the effects of the electric field in the optical response. The

critical electric field plays an important role in equalizing the linear and nonlinear

optical responses at a specific field of around

and it is an important feature of the

nonlinear response under the same conditions of temperature and frequency. There are

two critical fields, and in the nonlinear optical response at different

temperatures. Also, increasing the frequency or the temperature leads to an increase in

the critical field.

Finally, we have shown that BLG exhibits a strong nonlinear response in the

terahertz to far-infrared regime under an electric field of around V/cm. In

particular, a moderate field can induce the frequency tripled term to appear at room

temperature. This suggests a potential for developing graphene-based optical and

photonic applications.

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Chapter 5

5 EXPERIMENTAL TECHNIQUES

5.1 Introduction

The previous chapters in this thesis are devoted to the theory and quantitative

calculations that are needed for explaining the properties of graphene. In the major

part of this chapter, however, there will be a detailed review of the most important

principal experimental methods and the computational techniques used to measure

and analyze the samples prepared from graphene material. In addition, this chapter

deals contains a full presentation of the devices used to study transmittance spectra

and gives a description of how this equipment works. Electrical measurements were

particularly important for examination of samples. In addition, the cryogenic systems

that were used in the laboratory will not be neglected. The helium refrigeration

systems, capable of cooling to 12 K and 5 K, allowed automatic computer control of

the temperature, but were also linked with a thermal control system so that the

settings could be changed manually.

5.2 Bomem Hardware

This section will describe the spectrometer system used in the laboratory. The

Bomem DA8 Fourier transform infrared (FTIR) interferometer spectrometer model

was used in this work, because it is an extremely high performance system designed

to collect spectra that will detect the greatest number of transitions within the standard

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spectra and because it allows for measurements over a wide frequency range (4-50000

cm-1

) at temperatures between 4 and 300 K.

The other features that characterize this type of spectrometer and which can

provide measurements in the low frequency region under finite temperature are the

light source, the detector, the beam splitter, and the temperature controller. The

Bomem DA8 operates under an integrated vacuum system that is linked with pumps

working to evacuate the air from the device and the sample space. The light source

used in these experiments is a black body radiator (Globar) at ~100 W, and two types

of beam splitter, the KBr and the Broadband, were used for different ranges,

depending on the frequency region and the sample. The most common types of

detector and the one most sensitive in the terahertz to the far infrared range are the

bolometer and the mercury cadmium telluride (MCT) detector, respectively. The

Bomem FTIR spectrometer is equipped with a water cooling system. The details of

this FTIR spectrometer are shown in Figure 5.1, and the system may be divided into

three sections[144].

The first section (upper section) contains the light source, the beam splitter

compartment, and the motor scan system, which is most important for obtaining a

wide spectral range with high resolution. It depends on moving mirror that travels

during system scans.

The second section (middle section) contains the beam switching compartment,

the sample compartment, and the detector modules. The beam switching compartment

contains a rotatable plane mirror and two focusing mirrors that create two focused

beams in the sample compartment. There are also three parallel output beams, as

shown in Figure 5.2(a). The detector modules are located at the front of the

instrument, where each detector receives a one beam of the focused beams in the

sample space. Possible sources are an Hg lamp, a Globar, and a quartz lamp. In

addition, the spectrometer in the laboratory is equipped with a cryostat: a He flow

Janis STDA 100 (LN2 and LHe, 4 - 400 K)” [145].

The last section (lower section) contains the vacuum leads, the power supplies,

and the data processing and control electronics. The vacuum system is computer

controlled to keep the spectrometer free of air, which helps to reduce unwanted

absorptions that occurs with molecules or and prevents deterioration and

destruction of the KBR beam splitter. What might be considered another section is the

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computer system, which is connected with the spectrometer by Ethernet cable to

control and manage the operation of the system.

The precise location of the scanning mirror is determined by a helium neon laser

reflecting from the scanning mirror, and it can be identified by counting the number

of fringes. Furthermore, the white light source in the upper section of the spectrometer

is essential for identifying the zero path difference (ZPD) position and provides a

synchronization signal which allows interferogram measurements to be referenced to

a fixed mirror position. Figure 5.2 (b) displays the optical configuration of the

Bomem DA8 FTIR spectrometer

Finally, all of the above equipment and measuring methods work together to

yield information on the absorption and transmittance spectra of prepared samples. In

measurements, a beam from the radiation source (Globar) is sent through a series of

reflections and refractions as it encounters the mirrors, including the moving mirror in

the upper section. The light is then shed on the sample, where it is absorbed and

transmitted. The remaining light (which can be calculated mathematically through the

Beer-Lambert law, which will be mentioned later) encounters the detectors, which are

installed at the end of the light path and prepared to receive the beam. The results are

analyzed by sending the data from the detectors to a computer system to obtain all the

information and yield the full spectrum of the sample [144-147].

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Figure ‎5.1. The Bomem DA8 FTIR interferometer spectrometer.

Scan motor

Scan tube

Light Source

Beam splitter

Detector modules

Sample compartment

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Figure ‎5.2. (a) Middle section of the Bomem DA8 FTIR spectrometer containing the beam

switching compartment, the sample compartment, and the two detector modules. (b) Optical

Configuration of the Bomem DA8 FTIR spectrometer [144,145,147].

(a)

(b)

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It is worth mentioning that it is necessary to first choose the appropriate beam

splitter, light source, and detector, depending on the spectral range required,

temperature conditions, the sample type and other factors. So, we will talk about the

two kinds of beam splitter used in this experiment.

5.2.1 KBr Beam Splitters

A beam splitter is an optical device based on a mirror that is constructed in

different forms to be used to split a beam of light into two beams of light following

different paths. I addition, it is an intrinsic part of most interferometers. Potassium

bromide (KBr) is the most common material used in beam splitters, as it provides

good coverage in the mid-IR range, as well as significant coverage of a portion of the

near-IR region. The overall performance of the KBr beam splitter in the near-IR

region is, however, severely limited when compared to that of the near-IR quartz or

CaF2 beam splitters [148]. The KBr beam splitter has a published spectral range of

7800-380 cm-1

. In these experiments, the KBr beam splitter was used to measure

wave numbers above 500 cm−1

. The KBr beam splitter has high modulation

efficiency. In this type of beam splitter, it is best to have air evacuation from the

device to avoid damage or deterioration. The beam splitter also must be protected and

placed in a safe box in order to prevent scratching. It comes carefully packaged in

plastic boxes with silica gel, as the beam splitter absorbs water from the air. KBr

beam splitters are required for interferometers, autocorrelation, and laser systems

[148, 149].

5.2.2 Broad Band Beam Splitters

The Broadband beam-splitter has a newly developed coating which gives it

generally better performance over the spectral range from 50 to 500 cm-1

compared to

the previous technique used to cover this range, with four Mylar beam splitters 3, 6,

12, and 25 microns in thickness. Due to the coating technique, the physical properties

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of the Mylar substrate, and the coating, defects may be observed in the beam splitter.

Although the defects degrade the performance of the beam splitter compared to the

theoretical calculation, the practical performance is still superior to that of the bare

Mylar. Broadband beam splitters are delicate, and in order to obtain optimum

performance from the beam splitter, the manufacturer‟s advice on care, maintenance,

and usage must be observed the following recommendations for special care and

usage should be followed: Do not touch the film. When the beam-splitter is not in

used, it should be taken out form the beam-splitter holder to release the extra tension

on the film. As well as, an optical filter should be used in the beam path of your FTIR

spectrometer to eliminate unwanted stray radiation outside the spectral range of

interest. Finally, if the beam incident on the beam-splitter is not uniform, special care

should be taken when performing the peaking-up adjustment on the beam-splitter. The

most efficient areas of the beam-splitter are the shiny areas in between lines [150].

Figure ‎5.3. Beam-splitter range in wavenumbers (cm-1).

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5.3 Bomem software

The above-mentioned spectrometer system is under computer control. The

communication between the PC and the Bomem spectrometer takes place through an

Ethernet communication protocol called PCDA. The Bomem spectrometer uses

Microsoft Windows as the operating system for its basic data acquisition program.

By clicking the PCDA icon, a window showing the current status and operation

condition of the spectrometer is displayed, as shown in Figure 5.4. And the program

tries to establish communication with the spectrometer and the DA Initialization

message is shown on the screen. Generally, the Bomem system will show

Spectrometer Ready when the spectrometer is connected otherwise after 10 seconds,

the system will show an error message if the PC is unable to connect with the

spectrometer, then arrange the files and all the variables and parameters to be ready to

work as described in the user guide that came with the device. The main control panel

window is responsible for display the status of the spectrometer and various signals

while the system is acquiring data.

On the screen will be displayed important information about the status of the

device such as, the interferogram signal (% analogue to digital conversion (ADC))),

the mirror position (with this number referring to the value of the optical path

difference, which is a function of the resolution setting), the pressures inside the

source and sample compartments, the status of the laser stability, and other important

information. In addition, the scan control group (in the same screen ) displays another

option enables to control the screen for example, abort (to cancel the acquisition and

reset the communication with the spectrometer), stop the current acquisition and start

the spectrometer scanning in local mode as showing in Figure (5.4). Also worth

noting, the resource selection part and the configuration dialog box are provided to

define the group of resources (filter, source, Beamsplitter, and detector), which are

responsible to control and enable to select the required resources for an experiment

and stores them in the configuration file.

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Figure ‎5.4. The PCDA Collect window showing the current status and operation condition of

the spectrometer.

The important things that must be followed to prepare the spectroscope within the

windows is to determine the vacuum modes (Evacuate, Purge and change sample),

Aperture (range from 0.5 to 10 mm), speed, number of scans and other. On the other

hand, has been linked the computer dominating the performance of the spectrometer

to another host computer by Ethernet cable to analyze the results by using a program

called Igor Pro. Where, the results are converted and graphics by using Fourier

transformations to get the full spectrum of the sample and analyze data and graphical

and a comparison between the background and the sample spectra in standard

conditions. The program Igor Pro lets high and wide possibilities to deal with the data

supplied by the mother computer and through the results can get to the final results of

the spectrum [151-153].

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5.3.1 Interferogram analysis and Fourier transforms

In the beginning we clarify the meaning of FTIR, which means Fourier transform

infrared, which is the preferred method for spectroscopic analysis in the infrared

range. Fourier transforms are important for many mathematical and physical

applications in calculation and analysis of mathematical equations, such as in

quantum mechanics, image processing, solving boundary value problems on bounded

intervals by using Fourier series. This section will focus on one of the most important

interferometer designs, which is the well-known Michelson interferometer, as shown

in Figure 5.5(a), to describe Fourier transform spectroscopy (FTS) with the simplest

kinds of interference. In this the beam is divided into two paths of light by using a

beam splitter, and then the two beams are recombined after a path difference has been

introduced. "The variation in the intensity of the beams passing to the detector and

returning to the source as a function of the path difference ultimately yields the

spectral information in a Fourier transform spectrometer”. [154], This can be achieved

through a mathematical technique called the Fourier transformation by using the

computer linked with the FTS spectrometer which can calculate the desired spectral

information for analysis. Theoretically a symmetric shape around the zero path

difference (ZDF) should be observed, as shown in Figure 5.5(b), but in reality, an

asymmetric interferogram can be introduced by a phase error or phase shift (as shown

in Figure 5.5(c)). The main phase error contribution comes from the different optical

retardation in the beam-splitter plate compared with the compensator plate as a

function of wavelength due to thickness mismatch of both the substrates, but the

phase error does not destroy the spectral information [151-153]. Also, the

asymmetrical interferogram is shifted by an amount depending on the frequency.

Finally, Fourier transformations have come into greater use due the significant

changes in the process of spectral analysis in the infrared range, which made it

possible to develop many of the techniques that were difficult to achieve by older

techniques.

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Figure ‎5.5. (a) Michelson interferometer. The results can be (b) a symmetrical interferogram

and (c) an asymmetrical interferogram.

(b)Symmetrical Interferogram (c)Asymmetrical Interferogram

Detector

Movable Mirror

Direction of Travel

Source

Fixed Mirror

Beam-Splitter

Sample Position

(a)

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5.3.2 Definition of Fourier transforms theory from a

mathematical viewpoint

In this section, we will give brief a theoretical overview of Fourier transform

spectroscopy. FT spectroscopy is a technique for the rapid, accurate, and detailed

spectral analysis of electromagnetic radiation [154]. The best way to understand the

Fourier transformations is by using the mathematical analytical basis to reach an

understandable mathematical explanation. Therefore, we will consider the Michelson

interferometer, which can be called an “ideal” interferometer, as shown in Figure 5.5

[146, 154-156]. The Fourier transform is defined by the integral

{ },

where is known as the forward transform or Fourier transform

{ }.

The operation is called the inverse Fourier transform. The Fourier transform

pair can be formed for any variables, as long as the product of their dimensions is one,

Consider two electromagnetic waves, and , separated by a path difference

. The waves can be expressed as

∫ [[

The combination of these two waves represents the superposition and can be

rewritten as

∫ [

]

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On the other hand, the radiation incident on the ideal design can have intensity .

The intensity has the following relationship to the electric field

Here, < > is a time average and the electric field [

] Then, the intensity is obtained as follows

where c is the light velocity and is the permittivity of free space. So, we can

rewrite the above intensity as follows

[ ]

Now we can expand the intensity of the incident beam incident from the zero path

difference between those two split beams, i.e., t rearranging as follows

.

The broadband intensity can be written as

Finally, we can sum all the above to obtain the intensity as a Fourier transform,

yielding the ideal interferogram below

∫ [

]

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5.4 Optical Cryostats

The cryostat is a device to keep a sample at a required temperature for a period of

time sufficient to observe the operation. Therefore, the sample and the coolant should

be thermally isolated from their surroundings as much as is practically possible. The

sample and coolant are enclosed in a vacuum and surrounded by a radiation shield

[157-159]. A wide range of continuous flow cryostats is available. Some of these are

supplied with cryogens from a storage vessel; others are mounted in a bath cryostat

which supplies liquid. In most of these systems the cooling power available from a

flow of cryogen (LN2 or LHe) is balanced by power supplied electrically to a heater

near the sample (usually by a temperature controller). In this experiment cryostats

were used with liquid helium and had a temperature range from 4 to 300 K (see

Figure 5.6). Also, the temperature range can be extended to give lower temperatures

or higher, depending on what is necessary for the experiment. Conduction losses are

reduced by constructing the cryostat from low thermal conductivity material. “Static

systems are also fitted with heat exchangers, and the temperature of the heat

exchanger is controlled in a similar way. However, the exhaust gas does not flow over

the sample, but it passes out of the crystal to the pump through a separate pumping

line. The heat exchanger usually forms an annulus around the sample space, and

thermal contact is made to the sample through exchange gas. The exchange gas

pressure can be adjusted to suit the conditions.” [157-159]. The sample temperature

follows the temperature of the heat exchanger, but rapid temperature fluctuations tend

to be filtered out, and the temperature stability of the sample can be improved

considerably. In some cases, a heater is fitted to the sample block for fine control of

the temperature or to warm the sample quickly. Temperature control is achieved by

passing the cryogen through the heat exchanger.

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Figure ‎5.6. Optistat − an optical continuous flow cryostat [15].

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5.5 Detectors

Detector technology refers to techniques for measuring the radiation

transmittance of a sample over a wide range of frequency. Choosing the type of

detector to be used depends largely on the wavelength range and type of sample to be

measured. Thus, in this experiment, we used detectors that have a spectral range

extending from the terahertz to the far infrared. There are two main important types of

detectors, the thermal and the photonic. The thermal detectors can reveal the effects of

the incident IR radiation on different temperature dependent phenomena by using the

thermo-electric effect. Photonic detectors, however, have a sensitivity and response

higher than those of the thermal detectors, but these detectors must be cooled to

reduce thermal noise. In this section, we will discuss two types of detectors, one

thermal and the other photonic, which are the bolometer and the MCT, respectively.

5.5.1 Bolometer Detector

The response of the bolometer detector, which is cooled by liquid helium, is

based on changes in resistance. This type of detector has higher sensitivity from the

terahertz to far-infrared region than other detectors. The bolometer detector operates

between wavenumbers of 10 to 600 and yields its best performance in the far-

IR spectrum Fourier transforms (see Figure 5.7). The bolometer detector is based on

semiconductor elements and is used to measure the radiation energy. The way it

works depends on the change in temperature, when the electromagnetic beams are

incident on the sample and the infrared photons are absorbed, which leads to heating

of the sample and consequent changes in resistance, so that the detector is activated.

This detector has three types of filters, and whether to change or use those filters

depends on the required spectral range in the experiment, because each filter works

within a specific spectral range, as shown in Figure 5.8. This detector is costly

because it uses liquid helium [148, 160, 161].

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Figure ‎5.7. The bolometer detector.

Figure ‎5.8. Spectra of three types of filters in the bolometer detector [148,160,161].

Rela

tive

In

ten

sit

y (

Arb

itra

ry u

nit

s)

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5.5.2 MCT Detector

MCT refers to mercury cadmium telluride (MCT) detectors, which are

photoconductive detectors (see Figure 5.9). MCT detectors work the temperature of

liquid nitrogen and have an improved signal to noise ratio. They are considered one of

the best types of detectors for use in the mid-IR range. The MCT detectors are faster

and more responsive than other detectors which operate in the same range. They are

preferred for low energy measurements or for high speed kinetics. MCT detectors

operate in the wavelength range from 2 to 24 µm or for wavenumbers from 400 to

12500 They are designed for optimal performance in FTIR spectroscopy. This

detector is not costly because it uses liquid nitrogen [148,162, 163].

Figure ‎5.9. MCT detector [148,162, 163].

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5.6 Sample preparation

The samples used in the experimental part of this thesis work were Graphene, Si

A661 NTD, and Si A661 NTD coated graphene, where NTD represents neutron

transmutation doping. In our experiment, the sample preparation includes the

following steps. Firstly, we installed the sample on a special plate using phenyl

salicylate, which helps to paste the sample on the plate during cutting. Next, we used

a wire saw to cut the sample from the ingot. During the cutting, we used glycerine-

carborundum slurry (50 ml) with SiC (30 ml) and water (20 ml) to cut the sample

smoothly. Where the sample of silicon was cut, the dimensions were 13 mm to 12 mm

in length and 6 to 7 mm in width. Then, we refined and softened the surface of the

sample by using 1000 grit silicon carbide powder with water and by moving the

sample on the powder to erase saw marks. Next, we used alumina powder

micropolish from Buehler for polishing. To prevent Edser-Butler fringes, we wedged

the samples along their length during the polishing process.

The second step is coating the silicon with graphene. We used graphene liquid, as

shown in Figure 5.10(a). The silicon is dripped in graphene liquid and held at a

certain temperature until the water evaporates and the graphene is left on the top of

silicon surface. This is the reason why we polished one side of the silicon and left the

other side unpolished.

In the third step, both sides of the silicon are linked by an electrical cable

through the cryostat stick to measure the electrical current and resistance in limited

temperature and then connected this cable with the Source-Meter to To measure the

electrical properties, as will be explained in the next chapter. We used sharp scissors

for cutting the samples of graphene (pure graphene) accurately, while maintaining a

smooth edge. The samples were also installed on a transparent plastic plate to allow

them to be carried easily, and there was a hole in the middle of this plate to allow the

light to pass through the sample.

Figures 5.10(b) shows the pure graphene. Figures (a) and (b) shows the

dimensions of the silicon sample and the graphene-coated silicon used in the

experiment.

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Figure ‎5.10. (a) Graphene Oxide Liquid Crystals (Dispersion in water); (b) solid graphene

(Bends easily).

Figure ‎5.11. (a) Dimensions of silicon A661 NTD; (b) Silicon A661 NTD coated by

graphene.

(a) (b)

1.7

75

7m

m

Si A661 NTD

12 to 13 mm

Graphene

Diameter: 3.5 cm.

Thickness: 0.3 microns

Tensile modulus > 20 GPa

Color: Black

Aqueous dispersion: 250 ml

Concentration: 500 mg/L

Dispersibility: Polar solvents

Solvents: Water

Concentration: 4 mg/ml

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Chapter 6

6 Experiment

6.1 Introduction

In previous chapters, we studied the optical properties of single and

bilayer graphene theoretically. It is useful to study the optical properties

of graphene experimentally within a particular range of the spectrum from terahertz to

near-infrared through the far-infrared order to find the properties of this unique

material, based on the spectral behavior within this range of the electromagnetic

spectrum. The unique optical and electronic spectra of single layer graphene have

been studied most effectively by many researchers, both experimentally and

theoretically, due to its special features, which include the chemically strong

absorption lines and very good optical transparency in the visible and near-infrared

regions [164, 165].

The infrared (IR) frequency region is one those most commonly examined by the

spectroscopic techniques used by organic and inorganic chemists [166, 167].

Graphene is attractive for many scientists due to the strong vibrational modes in this

frequency region, indicating the physical properties of this carbon phase. So, the use

of the infrared region as a tool to explore this material has become very common.

Furthermore, the study of infrared spectra has acquired great importance in the

spectroscopy field for many chemical compounds due to the amount of information

that can be learned through their spectra. There are several major applications to

interpret the results of IR spectroscopy [168, 169] and Raman spectroscopy [170-

172], leading to extensive study of influences on atomic energy levels and atomic

vibrations, as well as helping to determine geometric forms and calculate the

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thermodynamic characteristics of molecules. To sum up, the study of IR spectroscopy

provides information on the inter- and intra-band transitions between the atoms and

various molecules [166,167,173,174]. The infrared frequency region of the

electromagnetic spectrum is divided into three regions, which are the near-infrared,

mid-infrared, and far-infrared, as shown in Figure 6.1.

On the other hand, terahertz spectroscopy offers unique applications and covers

an important area of the spectrum that adjoins the far-infrared. The terahertz

frequency region extends from 0.3 to 3 terahertz (THz) and is equivalent to energy of

about 4 meV and wave numbers of about 10 to 600 . The corresponding

wavelengths are from 1 mm to 100 μm, as shown in Figure 6.1. The intra-molecular

and inter-molecular transitions and vibrations in the atoms can be detected in the THz

region. In addition, most of the research work is within a specific area of the terahertz

range that extends only from 0.3 to 3 THz [175]. Therefore, in this work, we have

performed absorption and transmittance measurements on graphene from the terahertz

to the far infrared regime.

The mechanics of measuring absorption and transmittance can be defined through

the scheme shown in Figure 6.2. As it illustrates, the incident beam issues from the

source, which hits the surface of the sample. The beam passes through a series of

“mechanical” operations as in a so-called interferometer system, where part of the

incident beam is reflected from the sample and the other part is absorbed by the

sample after suffering a series of reflections inside the sample. Finally, some of the

incident light is passed through (transmitted through) the sample to meet the detector,

which will turn it into a spectrum through the principle of Fourier transforms. The

final spectrum can be used to read spectral information on the sample material. So, the

output spectrum represents the absorption and transmittance of the sample.

The main purpose of this chapter is measurement and analysis of the

transmittance and absorption in different type of graphene and graphene with silicon.

Firstly, the electrical effects were measured on the sample to examine the impact on

the sample of the voltages and currents at different temperatures (liquid nitrogen and

room temperature). Secondly, the effects of temperature on the absorbance and

transmittance peaks of graphene were verified, with and without silicon substrates. A

particular emphasis was put on the effects of the infrared beam on the transmittance

and absorption spectra in different samples and under different conditions.

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Figure ‎6.1. Schematic diagram of the electromagnetic spectrum.

Figure ‎6.2. Schematic diagram showing the mechanisms of reflection, absorption, and

transmission through the sample to produce the output spectrum.

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6.2 Electric measurements

In this section we proceed to measure the electrical effects on the samples by

applying a voltage to both poles of the sample and measuring the output current based

on the ratio between the voltage and current to define the value of the electrical

resistance, which is one of the most common quantities measured. So, the main

objective of this investigation is examining the electrical response and resistance for

all the samples at different temperatures and under different physical conditions. This

is because the behavior and electrical characteristics of the samples depend on the

temperature, which is changed by using liquid helium and nitrogen. In addition, the

physical properties of materials relating to temperature, pressure, and many other

conditions can be changed into electrical signals by using a power source.

In this experiment we measured the resistance by throwing infrared light on the

sample and applying a voltage to measure the output current at room temperature.

This system (shown in Figure 6.3) uses black-body radiation to generate infrared

beams. The beams are reflected from the mirrors to hit the sample, which is linked to

a Source-Meter, which changes the voltage and measures the current. The effects of

temperature on the resistance and the output current of the Pure Graphene was

measured by this method. Black polythene was also used to filter the IR beam, with

the light passing through the black polythene filter to hit the sample. Figure 6.3 shows

the simple system of optical and electrical management. It includes some optical and

electric equipment such as an infrared source (Globar), mirrors, a power supply, a

function generator, and other types. On the other hand, the sample space is evacuated,

and the sample can be subjected to high pressure. Helium and liquid nitrogen were

used to change the temperature in the cryostat to keep samples at the required

temperature.

In my experiments, the samples used for electrical tests were Si A661, Si A661

with Graphene and Pure Graphene. Figure 6.4 shows the current-voltage curves of Si

A661 with and without graphene. The current is a function of voltage at room

temperature under an infrared beam without any filter. Figure 6.4 shows that

increasing the voltage on the Si with and without graphene increases the current. We

note, however, that the rate of increase in current with voltage for just the silicon

substrate under the infrared regime is greater than for the rate of increase in silicon

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143

with graphene, which indicates higher resistance in the silicon alone than in the

silicon with graphene. This confirms that the electrical conductivity of graphene is

greater than that of silicon, since the resistance is inversely proportional to the

electrical conductivity.

Figure ‎6.3. Schematic diagram of the simple optical and electrical system to measure the

electrical resistance of the sample.

Figure 6.5 shows the current against voltage at room temperature with black

polythene filter in the path of the infrared beam. This figure also shows that the

current through Si with and without graphene increases gradually with increasing

voltage at room temperature. From a comparison between Figures 6.4 and 6.5, we can

note that with the black polythene filter, the current increases through the Si (with and

without graphene) as the voltage is increased, but the rate of increase with the filter is

less than without it. Furthermore, we can observe from both these figures that the

resistance of the Si without graphene exceeds that of the Si with graphene.

Figure 6.6, shows plots of the voltage dependent current of Si A661 with and

without graphene at nitrogen temperature. It indicates that the temperature has a very

strong effect on the resistance of both Si and Si with graphene.

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Figure ‎6.4. Current-voltage curves of Si A661 with and without graphene at room

temperature.

Figure ‎6.5. Current-voltage curves at room temperature for the Si substrate with and without

graphene film, with black polythene filter in the path of the infrared beam.

8

6

4

2

Vo

lta

ge

(V

) x

10

-2

10080604020

Current (A)x10-4

Si A661 NTD with Globar

Graphene on Si A661 NTD with Globar

Graphene on Si A661 NTD with filter

Graphene on Si A661 NTD without filter

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Figure ‎6.6. Voltage dependence of the current through Si A661 with and without graphene at

nitrogen temperature.

The correlation obtained between the temperature and the resistance of graphene

is demonstrated in Figure 6.7, where the voltage and resistance diminish progressively

with increasing temperature. Also, we can observe the stability of the voltage when

the temperature is increased by more than about 150 K. This stability depends on the

current changing. In addition, our analysis indicates that the temperature and current

affect graphene very strongly, and this Fig. 6.7 also shows that resistance is going to

be infinite at zero temperature because there are no free conduction electrons. For this

reason, the resistance will continue to decrease as the charge carrier density in the

conduction band increases. In addition, when comparing Figure 6.7 and Figure 6.8,

we note that there is negligible change between the sample of graphene with and

without the black polythene filter. Finally, Figure 6.9 shows the inverse relationship

between the resistance and temperature, and shows also the linear relationship

between the current and voltage of graphene at finite temperature. The value of the

electrical conductivity depends on the temperature, due to the exponential increase in

40

30

20

10

Vo

lta

ge

(V)

10

-2

10080604020

Current (A) 10-4

Si A661 NTD at Nitrogen Temperature

Si A661 NTD with Graphene at Nitrogen Temperature

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the number of electrons with temperature, meaning that the electrical conductivity

increases with temperature. The resistivity of metals increases with increasing

temperature, but the resistivity of Graphene usually declines as temperature is

increased because the temperature coefficient of resistance is negative for

semiconductors and insulators, while it is usually positive for metals

). The relationship between the temperature and

resistance can be explained as follows [176-178]:

(6.1)

[ ]

or

[

(

*]

Here, is the temperature coefficient of resistance, is a fixed reference

temperature, Boltzmann‟s constant, and is the resistance at temperature . So,

this is one of the features of graphene, that it has a low resistance at room

temperature.

Figure ‎6.7. Temperature dependence of the voltage under infrared radiation for Graphene for

different values of current.

200

150

100

50

0

Vo

lta

ge

(mV

)

30025020015010050

Temperature (K)

Graphene 519 Ag with infrared beam Current=0.3 (mA)Current=0.6 (mA)Current= 1 (mA)

Graphene

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Figure ‎6.8. Temperature dependence of the voltage of Graphene with and without infrared

radiation for 1 mA current.

Figure ‎6.9. Current dependence of the voltage of Graphene at different temperatures under

infrared radiation.

Graphene

Graphene

Graphene

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6.3 Theoretical model of transmittance and reflection

To study the reflection, absorption, and transmittance of light on a material and to

describe the optical properties of the medium, we will first consider the Fresnel

formulas to explain most of the optical information relating to the interfaces of the

material, where an interface is really a boundary with another medium with a different

refractive index. Secondly we will consider Snell‟s law to determine the angles of

incidence and refraction on a planar surface separating two different media with

approximately equal permittivity . The Fresnel formula describes

the behaviour of electromagnetic waves when moving between media of differing

refractive indices (from a medium with refractive index into a second medium with

refractive index ) and is an expression of the intensity of light reflected from the

surface of a dielectric, as a function of the angle of incidence, which depends on the

electric field and magnetic field. In addition, the Fresnel formula can be defined in

terms of the intensity of the electric field and magnetic field, as light is an

electromagnetic wave [179, 180].

The calculations of reflectance and transmittance depend on the polarization

of the incident light. There are two possibilities for the incident light, depending on

the angle of incidence as a function of the polarization of light with respect to the

electric field. First case: the incident light is polarized with the electric field of

the light perpendicular to the plane, as shown in figure 6.10.

Figure ‎6.10. The electric field of the light is perpendicular to the plane of incidence and the

magnetic field is parallel to it.

�� 𝑖 �� 𝑟

�� 𝑡

�� 𝑖 �� 𝑟

�� 𝑡

𝜃𝑖 𝜃𝑟

𝜃𝑡

�� 𝑖

�� 𝑟

�� 𝑡

Interface 𝑛𝑖 𝑛𝑟

𝑛𝑡

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The relation between electric field and magnetic field can be defined by

where is the wave speed. The continuity of the tangential component of the

E-field across the boundary at the interface between the media at any point is given

as:

(6.2)

Here, and are the incident, reflected, and transmitted light, and the

subscripted 0 refers to the amplitude of the wave equation for the light. The boundary

conditions require that the tangential component of the E-field and magnetic field in

both media ( at the interface must be equal. Therefore, the continuity of the

tangential component of the B-field across the boundary conditions at any point is

given as

(6.3)

Here, the effect on the B-field of the two media appears via their permeabilities

and .Equations (6.2) and (6.3) on both sides (the left-hand and right-hand) represent

the total electric field of E-perpendicular and the total magnetic field of -parallel

to the plane of incidence and the transmitting media, respectively.

Where

and the refractive index of the incident light equal the refractive

index of the reflected light i.e. ( ) and , so the above equation will be

rewritten as follows

substituting for by using Eq. (6.2). Then, we will rewrite the above equation

as follows in order to find the general reflectivity coefficient

(

* (

*

(

)

(

)

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Here, as most often happens with dielectrics. Therefore, the

equation for the amplitude of the reflection coefficient will be given as follows

(6.4)

By using Equations (6.2) and (6.3), we can calculate the equation for the

amplitude transmittance coefficient in that case and find , which is derived as

follows

Where , We substitute for in Eq. (6.2), so the above equation

will be rewritten as follows

(

*

(

)

(6.5)

Where we were assuming that . The equations of the amplitude

transmittance coefficient and of the amplitude reflection coefficient (Eqs. (6.4 ) and

(6.5)) for the electric field of light perpendicular to the plane are called the

Fresnel Equations for perpendicular polarized (s-polarized) light [179-182].

Figure ‎6.11. The electric field is parallel to the plane of incidence, and the magnetic field is

perpendicular to it.

�� 𝑖 �� 𝑟

�� 𝑡

�� 𝑖 �� 𝑟

�� 𝑡

𝜃𝑖 𝜃𝑟

𝜃𝑡

�� 𝑖

�� 𝑟

�� 𝑡

Interface 𝑛𝑖 𝑛𝑟

𝑛𝑡

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Second case: the incident light is polarized with the electric field of the light

parallel to the plane, while the magnetic field is perpendicular to it, as shown in Fig.

6.11.

In this case the continuity of the tangential component of the E-field across the

boundary conditions at the interface between the media at any point is given as [179-

182]:

(6.6)

The B-field across the boundary conditions at the interface between media at any

point is given as:

(6.7)

By following the same steps as above, we can derive the equations for the

amplitude transmittance coefficient and for the amplitude reflection coefficient when

the electric field lies parallel to the plane of incidence and the magnetic field is

perpendicular to it.

(6.8)

We substitute the existing value of in the Equation (6.6) into Equation (6.8).

Then, the above equation can be written in the following form

( )

Where the refractive index of the incident light equal the refractive index of the

reflected light, i.e , and , so the ratio between and is

defined as follows

(6.9)

In much the same way as before, the equation for the amplitude transmittance

coefficient can be derived by calculating the ratio between and from Equation

(6.8), where , which can be rewritten in the

following formula

(

* (

*

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Where , and , the above equation can be reduced to the

general form of

(6.10)

The equations for the amplitude transmittance coefficient and the amplitude

reflection coefficient (Eqs. (6.4) and (6.5)) under the electric field of light parallel to

the plane are called the Fresnel Equations for parallel polarized (p-polarized) light. It

is worth noting that the transmittance coefficient for parallel polarized (p-polarized)

light is similar to the transmittance coefficient for perpendicular polarized (s-

polarized) light, but this is not the same in the case of the amplitude reflection

coefficient [179-182].

Now, we have to employ the reflection coefficient equation to calculate the

reflectance and to find the relationship between them. In this case, the reflectance

formula will represent the ratio between the reflective power (Ir = reflected flux

density) and the incident power (Ii = incident flux density), which is given as follows

(6.11)

Where (6.12)

| |

(6.13)

| |

Here, and represent the cross-sectional areas of the incident and

reflected rays. Since and the incident ( ) and reflected rays ( ) are in the

same medium, the ray‟s area doesn‟t change on reflection, i.e. ( . In this case,

Equation (6.11) through Equations (6.12) and (6.13) leads to

(6.14)

| |

| | |

|

In normal incidence ( ), the reflectance equation will be given as

(

*

Where / . The above equation is the reflectance equation and also is

called the reflectivity equation (from the square of the reflectivity). In the same way,

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153

we have to define the transmittance as the ratio of transmitted power (transmitted flux

density ) to the incident power , which can be obtained as

(6.15)

(6.16)

| |

Through Equations (6.15) and (6.12), the transmittance equation can be expressed

by

(6.17)

|

|

(

*

Since / , and , this equation represents the transmittance

equation and can be called the transmissivity equation. In normal incidence (

), the transmittance equation will be given as

(

* (

*

The angles of incidence and refraction ’ w [182]:

√ √

Where / . Equations (6.4), (6.5), (6.9), and (6.10) can be rewritten by using

Snell‟s law and are given by

These equations represent the relationship between the Fresnel Equations and

Snell‟s law and represent the establishment of general equations for the reflection

coefficient and the transmittance coefficient in both cases (parallel polarized (p-

polarized) and perpendicular polarized (s-polarized) light) [179-184].

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6.4 Transmittance of single layer thin metal film

Understanding the optical properties of two-dimensional materials such as silicon

and graphene will depend on our ability to measure the electronic and optical

transitions and calculate the values for the reflection, absorption, and transmittance of

these materials under standard conditions. Therefore, in this section we will calculate

the optical mechanisms in single and multilayer systems to describe a material in

terms of its optical properties. Figure (6.12) shows the total transmittance from

multiple internal reflections. As was mentioned above, the transmittance is the ratio

between the transmitted power and the incident power. Also, the material has a

thickness and absorption coefficient , which will be taken into account in the

theoretical calculations. There is another parameter involved in the optical behaviour,

the reflectance. As shown in Figure 6.12, the reflectance can be determined at the first

interface from and the radiation reaching the second interface is

. These equations represent a part of the internal reflections and

transmissions that occur within the material [179, 185].

The multiple internal reflections and transmissions are illustrated in this Figure,

which are given as follows

(6.18) [

]

The above equation can be calculated by using a geometric series, where the form

of the equation is similar to the form below

6.19

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155

Figure ‎6.12. Transmission, reflection, and absorption for a single-layer thin film without a

substrate.

Where . So, we can rewrite Equation (6.18) by applying the

geometric series in Equation (6.19) as follows

[

]

(6.20)

*

+

In this case since the incident medium is air, so the reflectance is

expressed as

(

*

(

* (

*

(6.21) (

*

Where the refractive index for the material is the complex index of refraction and

is obtained as , where is the imaginary part of , called the extinction

𝐑 𝟏 𝐑 𝟐𝐈𝟎𝒆 𝟐𝜶𝒅

𝐈𝟎

𝐑𝐈𝟎

𝟏 𝐑 𝐈𝟎

𝟏 𝐑 𝐈𝟎 𝒆

𝜶𝒅

𝐑 𝟏 𝐑 𝐈𝟎𝒆

𝟐𝜶𝒅

𝐑𝟐 𝟏

𝐑 𝐈𝟎𝒆 𝟐𝜶𝒅

𝐑𝟐 𝟏

𝐑 𝐈𝟎𝒆 𝟑𝜶𝒅

𝐑𝟑 𝟏 𝐑 𝐈𝟎𝒆 𝟒𝜶𝒅

𝐑𝟒 𝟏

𝐑 𝐈𝟎𝒆 𝟒𝜶𝒅

𝐑𝟒 𝟏

𝐑 𝐈𝟎 𝒆

𝟓𝜶𝒅

𝟏 𝐑 𝟐𝐈𝟎𝒆 𝜶𝒅

𝑹𝟐 𝟏 𝐑 𝟐𝐈𝟎𝒆 𝟑𝜶𝒅

𝑹𝟒 𝟏 𝐑 𝟐𝐈𝟎𝒆 𝟓𝜶𝒅

𝑹𝟐 𝒏 𝟏 𝟏 𝐑 𝟐𝐈𝟎𝒆 𝟐𝒏 𝟏

𝑰𝒕 𝑰𝟎

𝐑𝟑 𝟏 𝐑 𝟐𝐈𝟎𝒆 𝟒𝜶𝒅

d

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156

coefficient, and can be given in terms of the absorption coefficient as [179, 184-

186,187]:

From this equation, we can say that both and depend on the wavelength

[187].

6.5 Transmittance through a single layer of thin metal

deposited on a substrate

The previous section described all the optical mechanisms (reflectance,

absorption, and transmittance) for two-dimensional materials with no substrate. In this

part, the optical behaviour of a thin film with a substrate is discussed, and the total

reflectance and transmittance of the whole sample structure are calculated, where the

sample has a multilayer structure consisting of the thin film, the substrate, and air. In

the present analysis, there are two condition of transmittance in this case, as shown in

Figures 6.13 and 6.14. In the first instance, we will ignore all reflectance that takes

place in the substrate (substrate/air interface) due to the thickness of the substrate,

which leads to decay and fading of the internal reflections. The transmittance through

the first interface (air/thin film) was given in the preceding section. By following the

same steps, we will calculate the reflectance and transmittance resulting from the

second interface (thin film/substrate) as follows [188-191]:

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157

Figure ‎6.13. Transmittance, reflection, and absorption for a thin film on a thick, transparent

substrate. The reflectance in the substrate is not included.

The multiple internal reflections and transitions due to the multilayer structure of

the sample are illustrated in Figure 6.13 and are obtained as follows

(

)

Where . By using the geometric series of Eq. (6.19), we can simplify

the above equation to the following formula

(6.22)

𝐈𝐓𝟏 𝐈𝐓𝟐 𝐈𝐓𝟑 𝐈𝐓𝐧

𝐑𝟏 𝟏 𝐑𝟏𝟐 𝟐𝐈𝟎𝐞

𝟐𝛂𝐝

𝐈𝟎 𝐑𝟏𝐈𝟎

𝟏 𝐑𝟏𝟐 𝐈𝟎

α

𝐑𝟐 𝟐 𝟏

𝐑𝟏𝟐 𝐈

𝟎 𝒆 𝟑𝜶𝒅

𝐑𝟐 𝟒 𝟏

𝐑𝟏𝟐 𝐈𝟎 𝒆

𝟓𝜶𝒅

d

x

𝐑𝟐𝟑 𝟏 𝐑𝟏𝟐

𝟐𝐈𝟎𝒆 𝟒𝜶𝒅

𝑹𝟑 𝟎

𝜶𝟐 𝟎

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Here, and is the absorption coefficient of the substrate. This

equation refers to the optical transmittance under the standard conditions of

temperature and pressure. So, the substrate of the sample has enough thickness to

allow us to ignore the reflectance and absorption that occur within it.

In the second instance, we will take into account all the reflectance, absorption,

and transmittance, including what occurs within the substrate, as shown in Fig. 6.14.

where all the components of the optical transmittance for the first and second

interface of the metal are illustrated. Therefore, it is useful to define the optical

transitions and reflections within the substrate, as is shown in Figure 6.14 as follows

Figure ‎6.14. Transmittance, reflectance, and absorption of thin film on a thick, transparent

substrate. The reflectance in the substrate is included.

𝐑𝟐𝟑 𝟏 𝐑 𝟐𝐈𝟎𝒆

𝟒𝜶𝒅

𝐑𝟐 𝟏 𝐑𝟏𝟐 𝟐𝐈𝟎𝐞

𝟐𝛂𝐝

𝐈𝟎 𝐑𝟏𝐈𝟎

𝟏 𝐑𝟏𝟐 𝐈𝟎

α

𝐑𝟐𝟐 𝟏

𝐑𝟏𝟐 𝐈𝟎𝒆 𝟐𝜶𝒅

𝐑𝟐 𝟒 𝟏

𝐑 𝐈𝟎 𝒆

𝟓𝜶𝒅

𝑻𝟑

𝑻𝟏

𝑻𝟐

𝑻𝒏

d

x

β

𝑡

𝑡

𝑡 𝑡 𝑡

𝑟

𝑟

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159

So, the equation of the optical transmittance for the sample can be simplified

using an approximation based on the geometric series to solve an infinite series of

internal transitions within the sample, which can be written as follows

(6.23) (

)

So,

Here, ,

(6.24)

where and are the transmittance at the (substrate → air) interface and

the absorption coefficient of the substrate, respectively. and are small

under standard conditions. This means that the interface transmittance between the

substrate and air gives a negligible contribution to the total transmittance. Therefore,

Equation 6.24 can be rewritten as follows.

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160

(6.25)

Where

(

*

(

*

Then, we can rearrange Equation (6.25) as follows

(6.26)

In this equation, the optical transmittance does not include the angle of incidence

at the air → film boundary and does not involve the absorption of the substrate and

transmittance at the substrate → air boundary [190, 191]. Finally, these approximate

procedures usually are sufficient to determine and calculate T and R for a sample

which is composed of a thin layer placed on a substrate.

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6.6 Measuring the transmittance of silicone with and

without graphene.

The optical transmittance of thin films is very important for practical reasons,

because it primarily determines the optical properties and response of optical devices

such as THz and optoelectronic devices. Also, it provides significant information

about the internal transitions, absorption, and reflectance inside the samples. So, it is

worthwhile to conduct these investigations and determine the characteristics

experimentally for comparison with the theoretical results that we have reached in the

previous section. In this section, we will provide an experimental study of

transmittance, firstly, through silicon and secondly, through the silicon with a

graphene layer.

The following experiment was performed using a silicon A661 neutron

transmutation doped (NTD) [192, 193] sample under an infrared beam from a light

source (Globar). The Si sample was placed in a Fourier transform (FT) spectrometer

and was examined under appropriate conditions of pressure, temperature. etc., as

follows: temperature 300 K and pressure 0.2 Torr, with the spectrometer data set up

by computer, based on the following values: resolution , aperture , gain

200, and number of scans 1000. The spectral range extended from to

, depending on the type of detector and beam splitter used in the

experiment (bolometer and broadband, respectively, in this case). So, the filters in the

detector were changed depending on the range of the spectrum that was covered by

each filter to obtain a full and clear spectrum (see Chapter 5).

For the next step, after the completion of the spectroscope preparation, a

preliminary scan was made without any sample in the beam path, and then, after the

reference scan was complete, another scan was conducted on a sample of silicon

A663 NTD, Finally, the last scan was made on a graphene film placed on a substrate

of silicon A663 NTD. These tests on samples take a long time, depending on the

number and resolution of the scans. The final results are the spectra for the samples,

as shown in Figure 6.15.The as-obtained interferogram, however, will not be clear

enough to discuss and cannot be interpreted directly, and therefore, the Fourier

transformation was used. This was performed by computer, which then displayed the

spectral information on the sample, as shown in Figure 6.16.

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In the present measurements of the transmittance, the range of the spectra

( to ) was extended by using a mercury cadmium telluride

(MCT) detector and a KBr beam-splitter. The settings of the spectrometer were

preserved to conduct experiments on samples under similar conditions. Figure 6.17

presents the spectra of the transmitted radiation through the Si sample with and

without graphene, and the reference spectrum was collected with no sample in the

beam path.

In order to calculate the transmittance of samples, it is necessary to know the

theoretical definition, by which the transmittance is the ratio of the incident beam to

the transmitted beam. So, in our experiments, the transmittance was calculated by

taking the ratio between the background of the spectrometer (no sample in the path of

beam) and the transmitted beam through the sample. Figures 6.18 and 6.19, show the

transmittance ratio for silicon A661 NTD and graphene with silicon A661 NTD as a

function of the wave number (photon energy) in different detectors and beam splitters.

Figure ‎6.15. Raw spectra of the transmitted radiation through Si samples with and without

graphene.

800

600

400

200

0

-200

-400

-40x10-3 -20 0 20 40

Photon Energy (cm-1

)

21220.027

Glober, Bolometer, BrodBand, Res 4 cm-1, <0.20 Torr, Aprt 10mm, Gain 200, 300 K, 1000 scan

____Si A661 NTD ____Graphene on Si A661 NTD

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Figure ‎6.16. Spectra of the transmitted radiation through Si samples with and without

graphene, and the reference spectrum with no sample in the beam path (inset), using Fourier

transforms with bolometer and broadband beam splitter.

Figure ‎6.17. Spectra of the transmitted radiation through Si samples with and without

graphene, and the reference spectrum with no sample in the beam path, using Fourier

transforms with MCT detector and KBr beam splitter.

Rela

tive

In

ten

sity (

Arb

itra

ry u

nits) 1.4

1.2

1.0

0.8

0.6

0.4

0.2

0.0

800600400200

Photon Energy (cm-1

)

____Si A661 NTD

____Graphene on Si A661 NTD

Glober, Bolometer, BrodBand, Res 4 cm-1,<0.20 Torr, Aprt 10mm,Gain 200, 300 K, 1000 scan

60

50

40

30

20

10

0

10008006004002000

21220.021Glober, Bolo, BB, Rse 4cm-1, <0.39 Torr, Aprt 10mm,Gain 1*50*1, 300K, 100scan,Filter 1

No Samplein the beam path

Rela

tive

In

ten

sity (

Arb

itra

ry u

nits)

1.0

0.8

0.6

0.4

0.2

0.0

70006000500040003000200010000

Photon Energy (cm-1

)

____No Sample

____Si A661 NTD

____Graphene on Si A661 NTD

Globar, MCT, KBr, 0.5cms-1, 4cm-1,10mm apert, 2000scans, >0.3 torr, gain 200

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Figure ‎6.18. Ratio of the transmitted radiation through Si with and without graphene to the

reference spectrum with no sample in the beam path, with bolometer and broadband (BB)

beam splitter.

Figure ‎6.19. Ratio of the transmitted radiation through Si samples with and without graphene

to the the reference spectrum with no sample in the beam path, with MCT detector and KBr

beam splitter.

Tra

nsm

itta

nce

0.6

0.5

0.4

0.3

0.2

0.1

600500400300200100

Photon Energy (cm-1

)

Resolution= 9.0486 (cm-1

)

Glober, Bolo, BB, <0.19 Torr, Aprt 10mm, Gain 200, 300 K, 1000 scan

____Si A661 NTD

____Graphene on Si A661 NTD

Tra

nsm

itta

nce

0.30

0.25

0.20

0.15

0.10

0.05

0.00

600050004000300020001000

Photon Energy (cm-1

)

Resolution= 4.0028 (cm-1

)

Globar, MCT, KBr, 0.5cms-1,10mm apert, 2000scans, >1 torr, gain 200

____Si A661 NTD

____Graphene on Si A661 NTD

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6.7 Measuring the transmittance of Pure Graphene

The transmittance measurements of the Pure Graphene sample discussed in this

section was conducted by placing the sample in the path of the infrared beam in the

FT spectrometer and bolometer detector. For these measurements, the air was

evacuated from the sample place, and the spectrometer was kept under pressure (0.2

Torr). The samples were kept at 300 K temperature, and spectra were collected in the

range from 10 to 600 by using the broadband beam -splitter and bolometer

detector. In addition, this section presents a description of our experimental set-up and

storage of the data using computer programs. The experimental arrangement for the

Pure Graphene was the same as in our previous spectroscopy measurement for the

silicon and graphene with silicon. In the first step, we set up the spectrometer with the

following values: resolution , aperture , gain 200, and number of scans

1000 to 2000. In the first step, the FT spectrometer was scanned without any sample

in the path of beam. Thus, the first experimental result obtained here is shown in

Figures 6.20. In the next step, another scan was conducted with graphene. Here, the

experimental observation of the transmittance of the graphene, and the background of

the sample was done using the output spectrum of the Fourier transform technique.

The steps involved in this transformation is illustrated in Figure 6.21. The next step is

to cover the range of the electromagnetic spectrum from 400 to 6000 in

order to study the transmittance of graphene at long wavenumbers. This was done by

using the MCT detector and KBr beam splitter. Then, the spectrometer was set up

based on these new data, and the same conditions were maintained for the

temperature, vacuum, and pressure measurements. In much the same way as before,

the same steps were followed. Finally, the experimental observations of the

transmittance of the pure graphene was conducted using the ratio between the

background and the graphene spectrum with different detectors and beam splitters, as

shown in Figures 6.22 and 6.23. It is worth mentioning that the relative intensity may

not clear or be close to zero and disappear after nearly of the

wavenumber). So we've cut off the spectrum after this range in order to focus on the

important part of the spectrum.

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Figure ‎6.20. Raw spectrum of the transmitted radiation through Pure Graphene and with no

sample, using the bolometer and BB.

Figure ‎6.21. Spectrum of the transmitted radiation through pure Graphene and the reference

spectrum with no sample in the beam path (inset) using Fourier transforms with bolometer

and BB.

-10

-5

0

5

10

x1

03

40x10-3200-20-40

Photon Energy (cm-1

)

21220.026

Glober, Bolo, BB, Res 4 cm-1, <0.20 Torr, Aprt 10mm, Gain 200, 300 K, 1000 scan,

______No sample in the path of beam______Graphene (pure)

0.4

0.3

0.2

0.1

0.0

Re

lati

ve In

ten

sit

y

8006004002000

Photon Energy (cm-1

)

Graphene (pure) Glober, Bolo, BB, Res 4 cm-1, <0.28 Torr, Aprt 10mm, Gain 1*200*1, 300 K, 1000 scan, R

ela

tive

In

ten

sity (

Arb

itra

ry u

nits)

80

60

40

20

0

10008006004002000

No Sample in the path of beam

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Figure ‎6.22. Ratio of the transmitted spectrum through pure graphene to the reference

spectrum with no sample in the beam path, with bolometer and BB.

Figure ‎6.23. Ratio of the transmitted spectrum through pure graphene to the reference

spectrum with no sample in the beam path, with MCT detector and KBr beam splitter.

0.14

0.12

0.10

0.08

0.06

0.04

0.02

0.00

Tra

nsm

itta

nce

1400120010008006004002000

Photon Energy (cm-1

)

Glober, Bolo, BB, Resolution 4 cm-1,<0.28 Torr, Aprt 10mm, Gain 200, 300 K, 1000 scan,

Tra

ns

mit

tan

ce

3.5

3.0

2.5

2.0

1.5

1.0

0.5

0.0

x10

-3

140012001000800600

Photon Energy (cm-1

)

Graphene in the path of beam Globar,KBR,MCT,

Resolution= 4.0376 (cm-1

)

scans9000,Apert. 10.0mm,Gain 100x128, <1.00 torr

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6.8 Results and Discussion

The transmittance and reflectance described in Equations (6.20), (6.22) and (6.26)

can be determined as a function of wavenumber using the frequency range from the

infrared to the THz. Firstly, it is necessary to calculate these equations and plot the

theoretical results. In the experimental results, as shown in Figure 6.24 by calculating

the ratio of the beam transmitted through the sample (silicon and graphene on silicon)

to the background beam, the significant results were obtained when compared with

our theoretical calculations, within the wavenumber region that extends from 10 to

4000 .

Theoretical part: This calculation used the Fresnel formula to calculate the

transmittance and reflectance coefficient on the boundary between graphene and

silicon and between air and graphene based on the complex refractive index of

graphene: . Then, this result was fitted to the experimental spectra as a

function of wavelength or wavenumber, as shown in Fig. 6.24, where the complex

refractive index of the single layer and multilayer can be define as

[194, 195]. Here, [194, 195] in the visible range, but in our

measurement, we used the equation below to calculate (the extinction coefficient )

and C as follows [195]

6.27

(

)

where is the thickness of the graphene sheet, the wavenumber, the value of

and the value of is dependent on the wavelength and agrees with

the experimental part, where in the visible range [194, 195], however,

our experimental and theoretical results proved that the refractive index in the

frequency range from the terahertz to the infrared nearly equal and

.

It is worth mentioning that the absorbance of the silicon substrate is neglected in

the theoretical calculations because it is very small, and also, the internal reflectance

has been neglected due to the large thickness.

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Figure 6.24 shows the transmittance through the graphene on the Si sample

(black with blue fitting curve) and through the Si substrate (red with green fitting

curve), and the results include the multiple reflections from the front and back side of

these materials. Also, the reflectance at the interface of the graphene and the

absorption of the grapheme are included, where . In our

experiments, we can confirm that the graphene has absorption and reflectance of

approximately 20% (absorption and reflectance ), when

taking the ratio between the graphene on the silicon substrate sample and the silicon

only as a reference spectrum. In addition, we note the relation between the

transmittance and the wavelength, where increasing the wavelength leads to increases

in the transmittance spectrum. Also, the shifting of the wavelength from longer waves

to shorter waves (blue shift) causes the transmittance spectrum to decrease. It is worth

mentioning also, the number of layers depends on the rate of transmittance and

absorption and it is represent a few layers approximately less than 10 layers.

Figure ‎6.24. Experimental transmission spectra and the theoretical curve fitting results for

graphene on silicon and Si only.

0.5

0.4

0.3

0.2

0.1

0.0

600050004000300020001000

Photon Energy (cm-1

)

Curve Fit ResultsSun, 2 Jun 2013 2:12:28 AM

Fit Type: least squares fitFunction: Fit3Model: fit_BSpec13124007.IGMY data: root:'BSpec13124007.IGM'X data: _calculated_Coefficient values ± one standard deviation

n =3 ± 7.58e-154d =1.65 ± 0a =0.000574 ± 0

Curve Fit ResultsSun, 2 Jun 2013 2:00:22 AM

Fit Type: least squares fitFunction: FitT2Model: fit_BSpec13124005.IGMY data: root:'BSpec13124005.IGM'X data: _calculated_Coefficient values ± one standard deviation

n =3.3 ± 3.13e-158K =1.7 ± 0d =3.15e-005 ± 0b =1.65 ± 0

Si A661 NTD (Theoretical)

Si A661 NTD (Experimental)

Graphene on the Si A661 NTD (Theoretical)

Graphene on the Si A661 NTD (Experimental)

Tra

ns

mit

tan

ce

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It is worth to mentioning that the graphene on Si loses more than 60% of the

energy as a result of reflection from the first and second surfaces of graphene and of

the absorption of some incident beams as a result of interband and intraband

transitions between the energy levels of graphene. In the experimental analysis, the

sample consists of the four interfaces (air → graphene → Si → air), so this was taken

into account when conducting theoretical calculations. Here, the results confirm the

convergence with the theoretical results in the entirety of the thin film of silicon and

of the silicon thin film with graphene. We do not deny that there is a slight difference,

however. This is because we have neglected some weak transitions and random

defects on the back of the silicon or at the silicon → air interface (and the reflectance

from the interface polishing of the silicon substrate). So, there is a great convergence

between these results.

These results confirm that for the thin film of silicon and silicon with graphene,

absorption of the THz to infrared beam by the multilayer graphene occurs through the

multiple interactions with the graphene/Si interface and by the multiple internal

reflections within Si. Therefore, the transmittance of the graphene with the silicon is

less than for the silicon substrate.

Figure 6.25 shows the experimental spectrum of the transmitted radiation through

the multilayer graphene sample (red) and the theoretical transmittance of graphene,

which is fitted from 10 to 1000 cm-1

at room temperature (blue), where the

transmittance spectrum might disappear at short wavelengths (after ). As

can be seen in this figure, the theoretical model of the transmittance ratio for

multilayer graphene (graphite) shows a good agreement with the experimental results.

Furthermore, we can observe the decrease in the transmittance with increasing

number of the layers of graphene or thickness of the sheet of graphite. Due to that, the

opacity to light will increase linearly with increasing thickness of the sheet, and that is

consistent with our theoretical analysis [33].

In addition, the transmittance decreased at high energy and low wavelength that

means the shifting of the wavelength from longer waves to shorter waves (blue shift)

causes the transmittance spectrum to decrease (checking Figure 6.1 Schematic

diagram of the electromagnetic spectrum) due to the fact that the increase in

transmittance is due to the drop in interband conductivity. Also, the optical and

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infrared excitations, for example, often lead to interband transitions. that leads to

obstruct transmittance within the limited range of infrared. On the other hand,at low

photon energies (in the far-infrared spectral range) the optical absorption in graphene

is dominated by intraband transitions [198, 199].

Finally, there are many parameters that could control the transmittance through

the graphene and graphite such as the absorption, internal reflectance, and the

thickness of the graphite sheet in the sample or of the substrate, as well as the light

wavelength and complex reflective index, while the reflectance and transmittance also

depend on the polarization of the incident beam [179,196]. We would like to also note

that the interaction between the first graphene layer and the Si substrate is very much

stronger than for the second layer and above, and therefore, this layer will be a buffer

to reduce the effects that the substrate exerts on the other layer [33,197]. Also, that is

correspond with theoretical analysis.

Figure ‎6.25. Experimental transmission spectra and the theoretical curve fitting results for

pure graphene multilayer.

Pure Graphene (Theoretical)

Pure Graphene (Experimental)

0.14

0.12

0.10

0.08

0.06

0.04

0.02

0.00

Tra

nsm

itta

nc

e

1400120010008006004002000

Photon Energy (cm-1

)

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On the other hand, high optical transmittance of graphene and graphite can be

achieved due to the behaviour of carrier mobility of graphene at room temperature

and the low sheet resistance. These features can improve the transmittance and make

graphene the best candidate for transparent conductive electrode. The low resistivity

of our samples might open the way for carrier mobility to play an important role in the

transmittance and absorption.

At the beginning of the long wavelength range of the experimental measured

transmission spectra in Figures 6.24 and 6.25, there is deviation from the theoretical

predictions for wavenumbers shorter than 1000 cm-1

. The deviation is at a minimum

for graphene on silicon substrate and corresponds to 5 to 8 % less transmittance and

more absorption at 500 to 1000 compared to the present calculations and

theoretical fitting. The reasons for this deviation are not very clear. There are many

factors that may be responsible for this loss of transmittance. One of these, the

absorption and the scattering of light, may have increased for the sample at long

wavelengths [194-196]. Also, the sensitivity of the detector may be not adequate for

measuring at low energies and long wavelengths [148, 160, 161]. The overall

behaviour of the transmittance spectrum remains identical with the predictions of the

theoretical study, however.

the theoretical calculation is very useful for thick films, and when the distance or

thickness of the sample is greater than the wavelength, and when the value of

absorption or thickness is large, in the transmittance equation for graphene, only

the second term in the denominator can be neglected, and we can rewrite the equation

as follows [185].

(6.28)

Finally, we can confirm many of the important results achieved from our

experimental measurements and theoretical analysis of transmittance through

graphene, most importantly, that graphene possesses properties that qualify it as an

alternative for many of the materials used in optical instruments within the infrared to

THz range.

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6.9 Conclusion

The high transmittance and low resistance of graphene layers has prompted a

large number of experimental and theoretical investigations to investigate the

suitability of graphene for many applications such as transparent electrode. These

features were the motivation to study the transmittance and resistance in various

forms of graphene multilayers (in both standalone samples and samples placed on a

substrate). In conclusion, we have measured optical transmittance spectra through

graphene deposited on silicon substrate, multilayer graphene (graphite), and silicon

A661 NTD for a wide range of wavelength extending from the terahertz to the

infrared range. The experimental results have been shown to be in agreement with our

theoretical analysis, although there is a slight deviation at the long waves with low

energy.

Our results confirm the Fresnel model dependence of the absorption and inter-

and intra-band reflections of graphene and the dependence on the number of layers in

the terahertz to infrared frequency range, although our analysis does not take

transitions and reflections that occur within the substrate perfectly into account, thus

making it somewhat inaccurate at low energy and long wavelengths. Nevertheless,

our theoretical analysis showed a convergence with experimental results that was

greater than for the classic technique that does not consider internal reflections in the

substrate.

The achievement of the transmittance (increase or decrease) from the terahertz to

the infrared range in the multilayer sample (graphene on Si A661 NTD) and single

layer samples (graphene or silicon A661 NTD as a reference only) under

consideration at room temperature was feasible and useful due to the high mobility of

electrons in graphene at room temperature. Furthermore, one of the most commonly

used methods to analyse the spectra of samples is the Fourier transformation, and this

was suitable for use in this experiment.

Our results presented here indicate that FT spectroscopy can be used as the best

technique to describe the transmittance of graphene and graphite films and find the

values of parameters such as energy dispersion, absorption, reflectance, the complex

refractive index, and the number of graphene sheets. In this technique, a bolometer

with a broadband beam splitter and an MCT detector with a KBr beam splitter were

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174

respectively used in order to cover the largest area from the terahertz to the infrared

frequencies, where measurement of the optical transmittance spectrum over a long

frequency range can give useful information about the graphene structure. In addition,

there are also significant effects of pressure and vacuum towards improving the signal

and reducing the noise in the interferometer system.

In the present results, note that many of the following facts are confirmed through

experimental measurement and theoretical analysis: (i) The graphene multilayer on Si

substrate has low resistance at room temperature, less than the silicon alone, due to

the higher electrical conductivity of graphene. (ii) The graphene resistance is affected

by the temperature, so that increasing the temperature diminished the resistance, and

this is one of the very important features that characterize graphene as opposed to

other materials. (iii) Also, the results showed that the resistance of graphene with and

without Si substrate might be increased by using a black polythene filter for the

incident beam and decreased again without the filter. (iv) From our results, we

suggest using our method to calculate the transmittance and reflectance through

multiple layers because it is more accurate than the classic method, in that we have

included in our calculation the small reflections that occur in the substrate. (v) The

theoretical and experimental results also showed a good convergence at short and long

wavelengths. The transmittance increased toward long wavelengths, and while simple

deviations appeared, they did not violate the general trend of the spectrum. (vi) It is

worth noting that the transmittance can be affected seriously by the number of

graphene sheets and decreases linearly with increasing number of layers, leading to

increased absorption, which is inversely proportional to the transmittance.

Finally, in this chapter, the optical properties of graphene-based materials have

been shown to be quite important, diverse, and strong. The transmittance and

absorption of graphene represent a remarkable result in its own right and can be used

for terahertz application and for optoelectronic devices.

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Chapter 7

7 Conclusion

In the first part, the theoretical part, the optical response and electronic properties

of single, bilayer, and multilayer graphene in the terahertz to infrared regime form the

main objective of in this thesis in the first, second, third, and fourth chapters, which

embody the theoretical calculations. The linear and nonlinear optical conductivity of

single layer graphene is also studied in this thesis and calculated by using different

methods and approaches. The theory of the unique and various characteristics and

properties of graphene is presented in this thesis, in such aspects as photon-mixing,

the p-n junction, optical conductivity, optical transmittance, etc.

The Boltzmann equation and quantum theory have been employed to calculate

the optical conductivity of the gapless and gapped single layer graphene p-n junction

in the terahertz regime under electric field. The linear and nonlinear optical responses

of a single layer graphene p-n junction are dominated by nonlinear intraband and

interband transitions under a forward bias. At the experimentally relevant electric

field intensity, nonlinear conductance is an order of magnitude larger than the linear

conductance. Furthermore, the total conductance is negative in the terahertz to far

infrared regime.

The work outlined in this part indicates that this p-n junction could be used for

developing coherent terahertz radiation sources due to the following features that it

possesses:

1- The negative conductance of the gapped and gapless graphene p-n junction

provides a unique mechanism for photon generation in graphene.

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2- Negative conductivity is the result of the effect of bias voltage in the optical

response when

3- Opening a gap at Dirac cones, within a limited size, may contribute to

improvement of the optical conductivity of the p-n junction, where the band

gap provides an additional mechanism for tuning the position of the negative

conductance peak. In addition, the absence of the gap in graphene can be an

obstacle to other electronics applications. Graphene with a gap exhibits an

interesting optical response at low frequencies.

4- The negative optical conductivity of the p-n junction increases with

increasing relaxation time and bias voltage, and with decreasing temperature.

5- Under forward bias, the nonlinear optical response in the gapped graphene p-

n junction remains strong within the terahertz to infrared frequency range.

6- The effect of increasing electric field intensity leads to an increasing ratio of

the nonlinear to the linear optical conductance in the gapped and gapless

single-layer graphene (SLG), where the nonlinear optical conductance can be

an order of magnitude larger than the linear conductance when the electric

field intensity is on the order of .

7- Also, the ratio of the nonlinear to the linear optical conductance in the gapped

and gapless SLG decreases with increasing frequency.

8- Building in dual gate voltage on both sides (p-region) and (n-region) of the

junction can control the Fermi level of graphene.

During this work, the remarkable properties of gapped and gapless graphene-

based systems are proved theoretically through the photon-mixing process. The

nonlinear optical response over the full temperature spectrum of finite-doped ( )

gapless and gapped graphene monolayers has been calculated by using the quantum

mechanical approach with the tight binding model under both weak-field and strong-

field conditions in the terahertz to infrared regime.

The single layer graphene exhibits a strong nonlinear photon-mixing effect in the

terahertz frequency regime. The nonlinear current density in graphene increases with

increasing temperature, up to 300 K, and this can be stronger than the linear current

density under moderate electric field strength of approximately Due to

the exciting Dirac behaviour of the graphene quasi-particles, a low Fermi energy and

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177

electrons filling improve the nonlinear optical response under a strong field. In

addition, the optical nonlinearity of graphene can be affected more seriously by the

strong-field-induced Dirac fermion population redistribution and non-equilibrium

carrier heating.

In the present calculations, the Fermi-Dirac distribution in weak field (WDF) has

been used, as , but this will be different with the strong field (SDF), as

( ). This leads to the stronger nonlinear optical

response under SDF than under WDF. The nonlinear optical responses in gapped and

gapless graphene are affected by the strong field (SDF), however, there is no obvious

effect on the linear optical responses in gapless graphene under strong field compared

with the strong linear optical responses in gapped graphene under such a field.

From zero to finite temperature and under weak field, the nonlinear optical

response in gapped graphene is enhanced by approximately 8% over the nonlinear

optical response in gapless graphene, and it increases with increasing temperature

with a finite gap.

It is worth noting, in p-n junction and photon-mixing processes, that the second

order response is equal to zero in both the weak and the strong field regimes in

gapped and gapless graphene due to the inversion symmetry of the graphene structure.

Based on this work, doped graphene can potentially be utilized as a strong

terahertz photon mixer at room temperature. On the other hand, the band-gap opening

can affect the photon-mixing process, and the nonlinear current density in gapped

graphene is also improved, depending on the size of the gap and taking into account

the accuracy of the method by which it is engineered. Greatly increasing the band gap

in the graphene structure may lead to the destruction of many low lying states. At high

temperatures, the enhancement of the optical nonlinear response will not continue in

this regime.

The third part in the theoretical work in this thesis is focused on studying the

linear and nonlinear optical response of bilayer graphene by using the tight-binding

approximation near energy minima, especially in the important frequency regime of

terahertz to far-infrared, and through the Schrödinger time-dependent equation

including applied electric field. This equation also can describe the four energy bands

for bilayer graphene under the Fermi-Dirac distribution at finite temperatures.

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178

There are many interesting features which can be achieved by using bilayer

graphene:

Firstly, the first order linear optical conductivity is equal to 6 when the

frequency range is close to zero, and the second order is equal to zero due to time

reversal symmetry.

Secondly, the nonlinear effect is strong for a wide range of temperatures within a

specific range that extends from low to room temperature.

Thirdly, there are single frequency and frequency tripling nonlinear terms, the

latter of which is comparable to the linear term in the terahertz frequency regime and

under very moderate electric field. The field strength for the nonlinear effect in

bilayer graphene is well within the experimentally achievable range in laboratories.

Fourthly, increasing the temperature up to 300 K leads to a decrease in the optical

conductivity for electric field of 1000 V/cm. The linear conductance at low

temperature has less impact than the nonlinear conductance of , however, at low

temperature, the linear term is greater than the frequency tripled nonlinear response

within the same frequency range.

Fifthly, increasing the frequency leads to a gradual decrease in the nonlinear

optical response. Also, the single frequency nonlinear response is greater than the

frequency tripled nonlinear response in different frequency ranges.

In addition, the electric field strongly affects the optical response. The critical

electric field plays an important role in equalizing the linear and nonlinear optical

responses at a specific field of ~ . These results for bilayer graphene indicate

a potential for developing graphene-based optical and photonic applications.

The second part of this thesis is the experimental work, which includes two parts.

The sample preparation, devices used, and software programs are first presented.

The second part of the experimental work has two aspects. The first is the

presentation and investigation of the experimental results in the laboratory. The

second is the comparison of these results with the theoretical calculations of the

transmittance, absorbance, and reflectivity of the samples. Finally, by comparing the

theoretical results with the experimental results, the following conclusions can be

reached:

1- The Fresnel formula can be used to calculate the transmittance and

reflectance coefficient on the boundary between graphene and silicon, and

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179

between air and graphene based on the complex refractive index of graphene,

although this analysis does not take transitions and reflections that occur

within the substrate perfectly into account, thus making it somewhat

inaccurate at low energy and long wavelengths.

2- As result of the high mobility of electrons in graphene at room temperature,

study of the transmittance in the range from the terahertz to the infrared in the

multilayer sample (graphene on Si A661 NTD) and single layer samples

(graphene or silicon A661 NTD as a reference only) was feasible and useful.

3- Fourier transformation (FT) is found to be a useful method to analyze the

spectra of samples, and was very suitable for use in our experiments. In

addition, FT spectroscopy can be used as the best technique to describe the

transmittance of graphene and graphite films and find the values of

parameters. This technique used a bolometer with a broadband beam splitter

and an mercury cadmium telluride (MCT) detector with a KBr beam splitter

in order to cover the largest area from the terahertz to the infrared

frequencies. The use of pressure, vacuum, and other factors contributed to

improving the signal and reducing the noise in the interferometer system.

4- As one of the very important features that characterize graphene, graphene

multilayer on Si substrate has low resistance at room temperature, less than

that of the silicon alone as a result of the higher electrical conductivity of

graphene. In addition, increasing the temperature leads to decreasing

resistance.

5- From our results, we suggest using our method to calculate the transmittance

and reflectance through multiple layers because it is more accurate than the

classic method.

6- Comparison of the theoretical and experimental results showed good

convergence at short and long wavelengths.

7- Increasing the number of graphene layers had a strong effect on the

transmittance value. The transmittance decreased linearly with increasing

number of layers, due to the increase in the absorbance.

Finally, these results can be used to improve optoelectronic devices and could be

useful for new graphene-based optical devices and terahertz applications.

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