1 laser research institute university of stellenbosch simulation of nonlinear effects in optical...
TRANSCRIPT
1
Laser Research Institute
University of StellenboschWWW.LASER-RESEARCH.CO.ZA
Simulation of Nonlinear Effects in Optical Fibres
F.H. Mountfort, Dr J.P. Burger, Dr J-N. Maran
2
Outline• Introduction• The nonlinear Schrödinger equation• Terms of the nonlinear Schrödinger equation• Numerical method of simulation• Results
– Group Velocity Dispersion (GVD)– Self-Phase Modulation (SPM)– Combined GVD & SPM
• The Ginzburg-Landau equation• Conclusion
3
Introduction
• Potentially disruptive nonlinear behaviour• Accurately simulate all nonlinear effects• Design for high energy, ultrashort pulse fibre
amplifiers• Simulation involves numerically solving the
nonlinear Schrödinger equation by means of the finite difference method
4
The Nonlinear Schrödinger Equation (NLSE)
• Use Maxwell’s equations to obtain:
• But
• Hence
• Use slowly varying envelope approximation– Factor out rapidly varying time dependence
2 2
02 2 2
1
c t t
E PE
NLL PPP
2
2
02
2
02
2
22 1
tttcNLL
PPE
E
5
• Wave equation for slowly varying amplitude:– Work in Fourier domain → Factor out rapidly
varying spatial dependence– Ansatz:
• where– F(x,y) = modal distribution– = slowly varying function– = spatial dependence
• Use retarded time:
ziezyxFrE 000 ,~,,
~
0,~ z
gT t z v
zie 0
6
• Finally NLSE:
• In summary:– Maxwell equations NLSE:
• with a description of the the field in terms of a slowly varying amplitude
2
2
2
22
1
2
T
i
zi
7
Terms of the Equation
• Absorption : ; α = absorption coefficient
• Group velocity dispersion: ; β2 = GVD parameter • Self-phase modulation:
Where
area = effective area of the core n2 = nonlinear index coefficient k = wave number
2
i
2
2 2
1
2 T
2||
area
kn2
22
2 2
1
2 2
ii
z T
8
Numerical Method of Simulation
• Propagation of a pulse in time with propagation distance
• Moving time frame traveling with pulse– Enables pulse to stay within computational
window• Finite difference method employed• Difference equation used to approximate a
derivative
9
FIBRE
TIME TIME
Illustration of Task
10
Group Velocity Dispersion (GVD)• Neglecting SPM and absorption:
• Different frequency components of the pulse travel at different speeds
• Two different dispersion regimes:
– Normal dispersion regime: β2 > 0
– Anomalous dispersion regime: β2 < 0
– Normal regime: red travels faster blue– Anomalous regime: blue travels faster
2
2 2
1
2i
z T
11
Illustration Of Traveling Frequency Components
Propagation
Initial pulse Final pulse
•Time delay in the arrival of different frequency components is called a chirp
TIME TIME
12
GVD Cont.• For significant GVD: with
• Initial unchirped, Gaussian pulse:
• Amplitude at any distance z:
dL L
2
20
0, exp2
TT
T
20
1 22 0 22
0 2
, exp2
T Tz T
T i zT i z
20
2d
TL
13
1.5 2 2.5 3 3.5
x 10-11
0
0.2
0.4
0.6
0.8
Dispersion of the pulse with propagation distance
Time Span [s]
Nor
mal
ised
Inte
nsity
Pulse @ 0Ld
Pulse @ 2Ld
Pulse @ 4Ld
14
-5 0 5 10
x 1011
0
0.5
1
1.5
2
2.5
x 10-12 Numerical spectra of the pulse
Frequency [Hz]
Spe
ctra
l Den
sity
Spectrum @ 0Ld
Spectrum @ 2Ld
Spectrum @ 4Ld
15
Self-Phase Modulation (SPM)• Neglecting GVD:
• For SPM: with
• Amplitude at z:
• Where
• New frequency components continuously generated
• Spectral broadening occurs• Pulse does not change
2
2
ii
z
nlL L
, 0, exp ,NLz T T i z T
2, 0, eff
NLNL
zz T T L
1
0nlL P
16
2 2.2 2.4 2.6 2.8 3
x 10-11
0
0.2
0.4
0.6
0.8
1
Time [s]
Nor
mal
ised
Pow
erNumerical Powers of the Pulse
Pulse @ 0Lnl
Pulse @ 2Lnl
Pulse @ 4Lnl
17
-5 0 5
x 1012
0
0.5
1
1.5
2
2.5
x 10-12
Frequency [Hz]
Spe
ctra
l Den
sity
Numerical Spectra
Spectrum @ 0Lnl
Spectrum @ 2Lnl
Spectrum @ 4Lnl
18
SPM Cont.• The following should hold:
– Max Phase shift ≈ (No. of peaks – 1/2)π– Govind P. Agrawal. Nonlinear Fibre Optics. Academic Press, 2nd edition.
-5 0 5
x 1012
0
0.5
1
1.5
2
2.5
x 10-12
Frequency [Hz]
Spectr
al D
ensity
Numerical Spectra
Spectrum @ 0Lnl
Spectrum @ 2Lnl
Spectrum @ 4Lnl
19
Combined GVD and SPM
• For both GVD and SPM:
• Normal dispersion regime:– Pulse broadens more rapidly than normal– Spectral broadening less prevalent
• Anomalous dispersion regime:– Pulse broadens less rapidly than normal– Spectrum narrows
d nlL L
20
FWHM with propagation distance for different dispersion regimes
0 200 400 600 800 1000 12000
500
1000
1500
2000
2500
Distance [m]
FW
HM
[s]
Normal regimeAnomalous regimeNormal regime no SPM
21
Spectra in Normal Regime Spectra in Anomalous Regime
Frequency [Hz]
-5 0 5
x 1011
0
1
2
3
4
5
6
x 10-24
Inte
nsity
-2 0 2 4
x 1011
0
2
4
6
8
x 10-24
@ 0Ld
@ 1Ld
@ 2Ld
@ 3Ld
@ 4Ld
@ 5Ld
22
The Ginzburg-Landau Equation (GLE)
• This takes dopant into account
• Results do not agree exactly with published results of Agrawal– Govind P. Agrawal. “Optical Pulse Propagation in Doped Fibre
Amplifiers”. Physical Review A, 44(11):7493-7501, December 1991.
2 220 2 0
2 20 0
1
2 2
ig T gii
z n T n
23
My results
Agrawal’s results
-50
5
x 10-12
0
0
50
100
150
Time Span [s]
No
rma
lise
d P
ow
er
Ld
2Ld
24
Conclusion
• NLSE resuts in good agreement with previously published results
• Discrepancy exits with published results for GLE
• Future work:– Use C– Improve time and spacial resolutions– Collaborate with ENNSAT, France
25
Many THANKSTo
Dr J.P. Burger&
Dr J-N. Maran&