Superconductivity Lecture 1: Superfluidity, superconductivity, materials -Superfluidity and superconductivity -Materials, types of SC: conventional, heavy fermion, high T c Lecture 2: Microscopic properties, BCS theory -Pairing mechanisms: phonons, spin-fluctuations -BCS theory -Experimental Properties Dirk van der Marel Université de Genève 0
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Superconductivity · 624 CE, Brahmagupta in his book "Brahmasphutasiddhanta": "Make a wheel of light timber, with uniformly hollow spokes at equal intervals. Fill each spoke up to
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Superconductivity
Lecture 1: Superfluidity, superconductivity, materials -Superfluidity and superconductivity
-Materials, types of SC: conventional, heavy fermion, high Tc
Lecture 2: Microscopic properties, BCS theory
-Pairing mechanisms: phonons, spin-fluctuations -BCS theory
-Experimental Properties
Dirk van der Marel Université de Genève 0
624 CE, Brahmagupta in his book "Brahmasphutasiddhanta": "Make a wheel of light timber, with uniformly hollow spokes at equal intervals. Fill each spoke up to half with mercury and seal its opening situated in the rim. Set up the wheel so that its axle rests horizontally on two upright supports. Then the mercury runs upwards in some hollow spaces and downwards in some others, as a result of which the wheel rotates automatically forever."
In 1924 Albert Einstein and Satyendranath Bose predicted that cooling bosonic atoms to a very low temperature would cause them to fall
(or "condense") into the lowest accessible quantum state, resulting in a new form of matter.
There exists no classical explanation for the complete absence of friction in a superfluid
In 1938 Fritz London proposed BEC as a mechanism for superfluidity
in 4He and superconductivity.
5
4He atoms are Bosons
6
Bose-Einstein statistics
Numberofbosonsinstate k : Nk =
1e εk−µ( )/kBT −1
N bosons in a recipient of volume V Density : n=N/V
μ = chemical potential
μ self-adjusts such that
Nkk∑ =N
7
Fraction of bosons having εk ≠ 0 :
=ζ 3/2( )n!3
mkBT2π
⎛
⎝⎜⎞
⎠⎟
3/2
Remaining fraction N0/N = 1−N+/N : BEC
Bose-Einstein condensation
The fraction N+/N is proportional to T3/2 !
N+
N= 1
eεk/kBT −1k≠0∑
For k=0: Nk = ∞ Interpretation: N0 is a macroscopic fraction of N
At low temperatures : μ = 0 ⇒ Nk =1
eεk/kBT −1
8
T/T0
N0(T)/N
Bose-Einstein condensation
Condensationtemperature:kBT0=3.3125!2n2/3
m
N0N
=1− N+
N=1− T
T0
⎛
⎝⎜⎞
⎠⎟
3/2
Liquidhelium:n=2.2⋅1022cm−3⇒T0 =3.1K
9
Experimental λ point: Tc=2.3 K
315314 1010 −− << cmncm1995: Dilute cold atom gases. Wolfgang Ketterle ; Eric Cornell; Karl Wiemann
BECof87Rb
(web-siteNobelprize2001)
Bose-Einstein condensation
⇒0.5µK <T0 <2µK
10
Back to 1911
H. Kamerling Onnes�
Mercury
The discovery of superconductivity
11
Single-element superconductors
12
Thermodynamic properties: Specific heat jump at Tc
ZrB12
13
Magnetic properties: Perfect Conductor
⇒!∇×!E = m
ne2∂!∇×!j
∂t
⎫⎬⎪
⎭⎪⇒ ∂
!B∂t
= mne2c
∂!∇×!j
∂tFaraday:
1⎡⎣ ⎤⎦ !E = m
e2n1τ− iω
⎡
⎣⎢
⎤
⎦⎥!j
⇒σ ω( )≡!j!E= e
2nτ /m1− iωτ (opticalconductivity)
!∇×!E − c−1∂
!B /∂t =0
14
Perfect conductor: τ = ∞
⎫
⎬⎪⎪
⎭⎪⎪
⇒!E = m
ne2∂!j
∂t
Ampère'slaw:!j = c
4π!∇×!B⇒∇2 ∂
!B∂t
= 1λL2∂!B∂t
⇒∂!B x ,t( )∂t
=∂!B 0,t( )∂t
e− x/λL
⇒Deepinsidetheperfectconductor:∂!B/∂t=0
Magnetic properties: Meisner-Ochsenfeld effect (1933)
15
Perfectconductor:
!E = e−2mn−1∂
!j /∂t
∂!B /∂t =0
⎧⎨⎪
⎩⎪
Magnetic properties: Meisner-Ochsenfeld effect (1933)
Meisner&Ochsenfeld,deepinsidesuperconductor:!B =0
FritzLondon'shypothesis 1935( ):!j = − c4πλL2
!A
λL =mc2
4πnse2;ns = "superfluiddensity"
!E = −c−1∂
!A/∂t⇒ !E = 4πλL2∂
!j /∂t 1t Londonequation( )
!B =!∇×!A⇒
!B = − 4πc−1λL2
!∇×!j 2d Londonequation( )
16
Magnetic properties: Fritz London (1935)
!j = − c
4πλL2!A
2d Londoneqn: !B = − 4πc−1λL2!∇×!j
Ampère'slaw:!j = c4π!∇×!B
⎫⎬⎪
⎭⎪⇒
⎧
⎨⎪
⎩⎪
⇔ Superconductivity
⇓!B x ,t( ) = !B0 e− x/λL
Deepinsideasuperconductor
!B x ,t( ) =0
Ampère'slaw⇒!j x ,t( ) =0
0th Londonequation⇒ !A x ,t( ) =0 1t Londonequation⇒ !E x ,t( ) =0
∇2 !B = λL
−2 !B
17
Magnetic and AC properties of a superconductor:
LondonEquation:!js = −
nse2
m!A
A supercurrent can coexist with a normal current
Normalcurrent:!jn =
e2nn /mτ −1 − iω
!E ;nn = "normalelectrondensity"
Opticalconductivity:σ ω( ) =
!js +!jn!
E= c
2
λL2 πδ ω( )+ i
ω⎡
⎣⎢
⎤
⎦⎥+
τe2nn /m1− iωτ
Important consequences • An external magnetic field penetrates only within a surface layer of thickness λL • The supercurrent is confined to a surface layer of thickness λL • The magnetic flux through a superconductor is quantised in units of ϕ0=h/(2e)
ns(T) vanishes at Tc, and is maximal at T=0
18
Field- and current distribution inside a superconductor
E. F. Talantsev, A. E. Pantoj, W. P. Crum & J. L. Tallon,
Scientific Reports 8, 1716 (2018)
19
Magnetic properties: Types I and II superconductivity
20
Type I superconductivity
Type II superconductivity
Bc1 < B < Bc2 : Magnetic Flux Penetrates as Vortices Vortex: Angular momentum = ħ & Magnetic Flux = h/2e
Vortices interact with each other à Abrikosov vortex lattice
Magnetic properties: Type II superconductivity
21
Heavy Fermion Superconductors
Tc m*/m (from γ) CeIn3 0.2 K ~50 CeCu2Si2 0.7 K ~1000 CePt3Si 0.75 K ~400 CeCoIn5 2.3 K ~250 UPt3 0.48 K ~200 UBe13 0.85 K ~300 URu2Si2 1.3 K ~25 PuCoGa5 18.5 K ~80
F Steglich et al, PRL 43 (1979) 1892 A de Visser, A Menovsky, JJM Franse, Physica B+C 147, 81 (1987) MB Maple et al, PRL 56, 185 (1986) MJ Rice, PRL 20, 1439 (1968) K Kadowaki and SB Woods, Solid State Communications 58, 507 (�1986)
22
C=γT
ρ=AT2 γ=c’Ν(0) A=cΝ(0)2
1986: Possible High Tc Superconductivity in the Ba-La-Cu-O System
J.G. Bednorz and K.A. Müller Z. Phys. B - Condensed Matter 64, 189-193 (1986)
Karl Alex Mueller
J. Georg Bednorz
23
How to make a room temperature superconductor
24
RoomtemperatureSCexistsalready:NEUTRONSTARS
CassiopeiaAShterninetal:Tc>2’000’000’000K
Pageetal:Tc=500’000’000K
Toward superconductivity at room temperature
25
1987: Superconductivity at 93 K in a New Mixed-Phase Y-Ba-Cu-0 Compound System at Ambient Pressure
M. K. Wu, J. R. Ashburn, C. J. Torng, P. H. Hor, R. L. Meng, L. Gao, Z. J. Huang, Y. Q. Wang & C. W. Chu
PRL 58, 908-910 (1987)
1993: Superconductivity above 130 K in the Hg-Ba-Ca-Cu-O system A. Schilling, M. Cantoni, J. D. Guo & H. R. Ott
Nature 363, 56-58 (1993)
1993: Superconductivity above 150 K in HgBa2Ca2Cu3O8+δ at high pressures
C. W. Chu, L. Gao, F. Chen, Z. J. Huang, R. L. Meng & Y. Y. Xue Nature 365, 323-325 (1993)
2015: Superconductivity at 203 kelvin at high pressures (140 GPa) in sulfur hydride
AP Drozdov, MI Eremets, IA Troyan, VK Senofontov & SI.Shylin, Nature 525,73
Toward superconductivity at room temperature
28
Toward superconductivity at room temperature December 2018: SC at 250 K in LaH10 /170 Gpa �
AP Drozdov, PP Kong, VS Minkov, SP Besedin, MA Kuzovnikov, S Mozaffari, L Balicas, �F Balakirev, D Graf, VB Prakapenka, E Greenberg, DA Knyazev, M Tkacz & MI Eremets;
ArXiv:1812.01561
August 2018: SC at 280 K in LaH10 /202 GPa M Somayazulu, M Ahart, AK Mishra, ZM Geballe, M
Baldini, Y Meng, VV Struzhkin & RJ Hemley; �arXiv:1808.07695
29
220
240
260 LaH10 (170 GPa)
Toward superconductivity at room temperature LaH10 (202 GPa)
(140 Gpa)
30
Summary
31
• Superfluidity and superconductivity: Realisations of the perpetuum mobile
• Basic principles of Bose-Einstein condensation
• The discovery of superconductivity
• Meisner effect, type I superconductivity
• Fritz Londons’ interpretation of the Meisner effect
• Type II superconductivity and vortices
• Heavy fermion superconductors • High Tc and the quest for room temperature superconductors