Fiber Optical Communication Lecture 3, Slide 1 Lecture 3 • Dispersion in single-mode fibers – Material dispersion – Waveguide dispersion • Limitations from dispersion – Propagation equations – Gaussian pulse broadening – Bit-rate limitations • Fiber losses
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A definition of Fiber Optics - ttu.ee 3 - 2016.pdfIn the time domain the dispersed pulse is The output width (1/e-intensity point) broadens as Chirped Gaussian pulses (2.4.2) A Gaussian
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Fiber Optical Communication Lecture 3, Slide 1
Lecture 3
• Dispersion in single-mode fibers
– Material dispersion
– Waveguide dispersion
• Limitations from dispersion
– Propagation equations
– Gaussian pulse broadening
– Bit-rate limitations
• Fiber losses
Fiber Optical Communication Lecture 3, Slide 2
Dispersion, qualitatively
• Different wavelengths (frequency components) propagate differently
• A pulse has a certain spectral width and will broaden during propagation
The index of refraction as a function of wavelength
The dispersion in SMF (red) and different dispersion-shifted fibers
Fiber Optical Communication Lecture 3, Slide 3
Each spectral component of a pulse has a specific group velocity
The group delay after a distance L is
The group velocity is related to the mode group index given by
Assuming that Δω is the spectral width, the pulse broadening is governed by
where β2 is known as the GVD parameter (unit is s2/m or ps2/km)
Group delay, group index, and GVD parameter (2.3.1)
22
2
Ld
dL
d
dTT
d
ndn
c
d
ndn
c
n
cv
g
g
d
dL
v
LT
g
d
ndnng
Fiber Optical Communication Lecture 3, Slide 4
The dispersion parameterMeasuring the spectral width in units of wavelength (rather than frequency), we can write the broadening as
ΔT = D Δλ L,
where D [ps/(nm km)] is called the dispersion parameter
D is related to β2 and the effective mode index according to
The dispersion parameter has two contributions:
material dispersion, DM: The index of refraction of the fiber material depends on the frequency
waveguide dispersion, DW: The guided mode has a frequency dependence
2
2
22
1
2
2
2222
212,
2
d
nd
d
nd
vd
dc
d
dv
d
dcD
g
g
Fiber Optical Communication Lecture 3, Slide 5
Material dispersion (2.3.2)The material dispersion is related to the dependence of the cladding material’s group index on the frequency
An approximate relation for the material dispersion in silica is
where DM is given in ps/(nm km)
d
dnD
g
M
2
2
2
MMD 01122
Fiber Optical Communication Lecture 3, Slide 6
Waveguide dispersion (2.3.3)The waveguide dispersion arises from the modes’ dependence on frequency
n2g: the cladding group index
V: the normalized frequency
b: the normalized waveguide index
dV
Vbd
d
dn
dV
VbVd
n
nD
gg
W
2
2
2
2
2
2
2
2
V
22
1
2
2
2
1 anc
nnaV
21
2
nn
nnb
Fiber Optical Communication Lecture 3, Slide 7
Total dispersionThe total dispersion D is the sum of the waveguide and material contributions
D = DW + DM
Note: DW increases the net zero dispersion wavelength
The zero-dispersion wavelength is denoted either λ0 or λZD
An estimate of the dispersion-limited bit-rate is
|D|B Δλ L < 1
where B is the bit-rate, Δλ the spectral width, and L the fiber length
Fiber Optical Communication Lecture 3, Slide 8
The dispersion can have different signs in a standard single-mode fiber (SMF)
D > 0 for λ > 1.31 μm: “anomalous dispersion”, the group velocity of higher frequencies is higher than for lower frequencies
D < 0 for λ < 1.31 μm: “normal dispersion”, the group velocity of higher frequencies is lower than for lower frequency components
Pulses are affected differently by nonlinear effects in these two cases
Anomalous and normal dispersion
Fiber Optical Communication Lecture 3, Slide 9
Different fiber types• The fiber parameters can be tailored to shift the λ0-wavelength from
≈1.3 μm to 1.55 μm, dispersion-shifted fiber (DSF)
• A fiber with small D over a wide spectral range (typically with two λ0-wavelengths), dispersion-flattened fiber (DFF)
• A short fiber with large normal dispersion can compensate the dispersion in a long SMF, dispersion compensating fibers (DCF)
Dispersion compensating fiber
Fiber Optical Communication Lecture 3, Slide 10
Fibers in the labThis dispersion compensating module contains 4 km of DCF...
...and it compensates the dispersion in this 25 km roll of SMF
Fiber Optical Communication Lecture 3, Slide 11
Index profiles of different fiber types• Standard single-mode fiber
(SMF)
• Dispersion-shifted fiber (DSF)
• Dispersion-flattened fiber (DFF)
Fiber Optical Communication Lecture 3, Slide 12
Higher order dispersion (2.3.4)• Near the zero-dispersion wavelength D ≈ 0
– The variation of D with the wavelength must be accounted for
– We have used β2 = 0
• S [ps/(nm2 km)] is called the dispersion slope
– Typical value in SMF is 0.07 ps/(nm2 km)
3
32
2
2
d
dc
d
dDS
Fiber Optical Communication Lecture 3, Slide 13
Basic propagation equationWe will now develop the theory for signal propagation in fibers
The electric field is written as
• The field is polarized in the x-direction
• F(x, y) describes the mode in the transverse directions
• A(z, t) is the complex field envelope
• β0 is the propagation constant corresponding to ω0
Only A(z, t) changes upon propagation (described in the Fourier domain)
Each spectral component of a pulse propagates differently
)exp(),(),(ˆRe),( 00 tizitzAyxFt xrE
dtitzAzA
ziziAzA
)exp(),(),(~
)(exp),0(~
),(~
0
Fiber Optical Communication Lecture 3, Slide 14
The propagation constant• The propagation constant is in general complex
– α is the attenuation
– δnNL is a small nonlinear (= power dependent) change of the refractive index
• Dispersion arises from βL(ω)
– The frequency dependence of βNL and α is small
• We now expand βL(ω) in a Taylor series around ω = ω0 (Δω = ω – ω0)
1/vp 1/vg GVD(rel. to D) dispersion slope(related to S)
0
332210 ...,)(
6)(
2)()(
m
m
mLd
d
2/)()()(2/)()/)](()([)( 00 iicnn NLLNL
Fiber Optical Communication Lecture 3, Slide 15
Substitute β with the Taylor expansion in the expression for the evolution
of A(z, ω), calculate ∂A/∂z, and write in time domain by using Δω↔ i ∂/∂t
The nonlinearity is quantified by using δnNL = n2I where n2 [m2/W] is a
measure of the strength of the nonlinearity, and I is the light intensity
βNL = γ|A|2, where γ = 2πn2/(λ0Aeff) is the nonlinear coefficient
Aeff is the effective mode area and |A|2 is normalized to represent the power
γ is typically 1–20 W–1 km–1
Basic propagation equation (2.4.1)
AAit
A
t
Ai
t
A
z
ANL
262 3
3
3
2
2
21
Fiber Optical Communication Lecture 3, Slide 16
Basic propagation equation• Use a coordinate system that moves with the pulse group velocity!
– This is called retarded time, t’ = t – β1z
– We neglect β3 to get
• This is the nonlinear Schrödinger equation (NLSE)
– The primes are implicit
• The loss reduces the power ⇒ reduces the impact from the nonlinearity
• The average power of the signal during propagation in the fiber is
• Note: α is in m-1 while loss is often expressed in dB/km
AAAit
Ai
z
A
22
2
2
2
2
2/
2/
av
2
av )0(),(1
lim)(
T
T
z
TePdttzA
TzP
Fiber Optical Communication Lecture 3, Slide 17
Chirped Gaussian pulses (2.4.2)• To study dispersion, we neglect nonlinearity and loss
• The formal solution is
• Note: Dispersion acts like an all-pass filter
• We study chirped Gaussian pulses
– A0 is the peak amplitude
– C is the chirp parameter
– T0 is the 1/e half width (power)
02 2
2
2
t
Ai
z
A
ziAzA 22
2exp),0(
~),(
~
2
021
0 )/)(1(exp),0( TtiCAtA
00
2/1
FWHM 665.1)2(ln2 TTT
Fiber Optical Communication Lecture 3, Slide 18
• For a chirped pulse, the frequency of the pulse changes with time
– What does this mean???
• Study a CW (continuous wave)
– A is a constant
• Writing A exp(iβ0z – iω0t) = A exp(iφ), we see that ω0 = –∂φ/∂t
• We define the chirp frequency to be
– We allow φ to have a time dependence
– We get φ from the complex amplitude
• In this way, the chirp frequency can depend on time
– For the Gaussian pulse we get ωc = Ct/T02
Chirp frequency
)exp(),(),(ˆRe),( 00 tizitzAyxFt xrE
ttc /)(
Fiber Optical Communication Lecture 3, Slide 19
A linearly chirped pulseFrequency increases with time Frequency decreases with time
ωc ωc
tt
Fiber Optical Communication Lecture 3, Slide 20
Time-bandwidth productThe Fourier transform of the input Gaussian pulse is
The 1/e spectral half width (intensity) is
The product of the spectral and temporal widths is
If C = 0 then the pulses are chirp-free and said to be transform-limited
as they occupy the smallest possible spectral width
Using the full width at half maximum (FWHM), we get
)1(2exp
1
2),0(
~2
0
22/1
2
00
iC
T
iC
TAA
0
2
0 /1 TC2
00 1 CT
22
FWHMFWHM 144.012ln2
CCT
Fiber Optical Communication Lecture 3, Slide 21
We introduce ξ = z/LD where the dispersion length LD = T02/|β2|
In the time domain the dispersed pulse is
The output width (1/e-intensity point) broadens as
Chirped Gaussian pulses (2.4.2)
A Gaussian pulse remains Gaussian during propagation
The chirp, C1(ξ), evolves as the pulse propagates
If (C β2) is negative, the pulse will initially be compressed
C
i
bT
tiC
b
AtA
ff1
arctan22
)1(exp),(
22
0
2
10
)(sign
)1()(
)1()(
2
2
1
2/122
s
CsCC
sCb f
2/12
2
0
2
2
2
0
2
0
1 1)(
)(
T
z
T
zC
T
zTzb f
Fiber Optical Communication Lecture 3, Slide 22
Broadening of chirp-free Gaussian pulses
Short pulses broaden more quickly than longer pulses
(Compare with diffraction of beams)
2
2
0
2
2
11)(
T
z
L
zzb
D
f
Fiber Optical Communication Lecture 3, Slide 23
Broadening of linearly chirped Gaussian pulses
For (C β2) < 0, pulses initially compress and reaches a minimum at
z = |C|/(1+C2)LD at which C1 = 0 and
Chirped pulses eventually broaden more quickly than unchirped pulses0
2
0min
1
1
1
C
TT
Fiber Optical Communication Lecture 3, Slide 24
Chirped Gaussian pulses in the presence of β3
Higher order dispersion gives rise to oscillations and pulse shape changes
2
3
0
2
3
2
2
0
2
2
2
0
2
2
0
2
24
)1(
221
CLLLC2/00 T
Fiber Optical Communication Lecture 3, Slide 25
Effect from source spectrum widthUsing a light source with a broad spectrum leads to strong dispersive broadening of the signal pulses
In practice, this only needs to be considered when the source spectral width approaches the symbol rate
For a Gaussian-shaped source spectrum with RMS-width σω and with Gaussian pulses, we have
where Vω = 2σωσ0
2
3
0
3222
2
2
0
22
2
2
0
2
2
0
2
24)1(
2)1(
21
LVC
LV
LCp
Vω << 1 when the source spectral width << the signal spectral width
Fiber Optical Communication Lecture 3, Slide 26
If, as for an LED light source, Vω >> 1 we obtain approximately
A common criteria for the bit rate is that
For the Gaussian pulse, this means that 95% of the pulse energy remains within the bit slot
In the limit of large broadening
σλ is the source RMS width in wavelength units
Example: D = 17 ps/(km nm), σλ = 15 nm ⇒ (BL)max ≈ 1 (Gbit/s) km
Limitations on bit rate, incoherent source (2.4.3)
22
0
2
2
2
0
2 )()( DLL
)4/(14/ BTB
14 DBL
Fiber Optical Communication Lecture 3, Slide 27
In the case of operation at λ = λZD, β2 = 0 we have
With the same condition on the pulse broadening, we obtain
The dispersion slope, S, will determine the bit rate-distance product
Example: D = 0, S = 0.08 ps/(km nm2), σλ = 15 nm ⇒ (BL)max ≈ 20 (Gbit/s) km
Limitations on bit rate, incoherent source
22
212
0
22
3212
0
2 )()( SLL
18 2 SBL
Fiber Optical Communication Lecture 3, Slide 28
For most lasers Vω << 1 and can be neglected and the criteria become
Neglecting β3:
The output pulse width is minimized for a certain input pulse width giving