30.3.2006 funfacs meeting, toulouse 1 ustrat wp 1 theory wp 2
TRANSCRIPT
30.3.2006 FunFACS meeting, Toulouse 1
USTRAT
WP 1 Theory
WP 2
2
WP 1 Theory
1. Cavity solitons in a VEGSEL with frequency-selective feedback
P. V. Paulau1,2, W. J. Firth1, T. Ackemann1, Andrew Scroggie1,
A. V. Naumenko2, N. A. Loiko2
1Department of Physics, SUPA, University of Strathclyde, Glasgow, Scotland, UK2Institute of Physics, Academy of Sciences of Belarus, Minsk, Belarus3INFM, Como, Italy; 4 currently enjoying Italy
2. Master equation for describing VECSELs with intra-cavity elements
L. Columbo 1,3, A. Yao1, W. J. Firth1
3. A new method for adiabatic elimination
G.-L. Oppo1,4
3
CS in a VEGSEL
P. V. Paulau1,2, W. J. Firth1, T. Ackemann1, Andrew Scroggie1,
A. V. Naumenko2, N. A. Loiko2
1Department of Physics, SUPA, University of Strathclyde, Glasgow, Scotland, UK2Institute of Physics, Academy of Sciences of Belarus, Minsk, Belarus
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VEGSELTo keep things simple: only one complex equation for linearly polarized field
loss diffraction scaling phase-amplitudecoupling feedbackgain saturation
finite gain bandwidth
feedback: self-imaging, diffraction grating (envelope of filter: sinc-function) one round-trip in external cavity
note: there are no temperature effects in this model
we assume resonance in external cavity: 0 = m 2
5
Stationary states=0, only k = 0
supercritical bifurcation bistability between off-state and lasing states „old“ model with temperature: subcritical
Naumenko et al., Opt. Commun. 259, 823 (2006)
=0, with k > 0
bistability disappears no CS need for filtering
6
Structures with spatial filtering I
assume spatial filter in some Fourier plane in feedback loop
filter due to gain curve
spatial filter in feedback loop
=0
=0.06
f=0.06
f=0
f = 0.06
pattern forming instability
potential for CS
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CS
real part intensity far field
this is a localized traveling wave !
is exponentially localized exists on grids 64, 128, 256
energy=azimutally integrated intensity
r (pixels)
log
(e
nerg
y)
f = 0.06
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CS II
can exist at different locations in the plane
several LS can coexist
present or absent under the same conditions
seems to be a self-localized solution, a true cavity soliton
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Symmetric structurereal part intensity far field initial condition:
homogeneoushigh-amplitudestate on zero background
not a Bessel beam: energy decays exponentially
is this related to experiment ?
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CS for detuning zero !?
direct excitation of CS apparently not possible,but taking CS from f = 0.06 as initial conditiona localized solutions is obtained
f = 0
real part NF far field cut through FFazimutally averaged FF
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Summary: VEGSEL theory
very exciting result: localized traveling wave
symmetric and asymmetric
relationship with experiment unclear: temperature, spatial filter ....
need to translate to physical parameters
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Master equation
1Department of Physics, SUPA, University of Strathclyde, Glasgow, Scotland, UK3INFM, Como, Italy
L. Columbo 1,3, A. Yao1, W. J. Firth1
idea: derive a closed equation for dynamics of nonlinear non-plano-planar resonators by using ABCD matrix to decribe intra-cavity elements
benefits: ability to model complex real-world cavities (e.g. VECSELs)
address effects of small deviations from self-imaging condition in external cavity describe properly action of grating in VEGSEL significance for WP1 and WP2
Dunlop et al., Opt. Lett. 21, 770 (1996)
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Thin lens::focal length=f
Nonlinear medium:Vapour of two levels atoms
Reference symmetric plane
PerfectMirror
PerfectMirror
Master equation for an unidirectional square nonlinear resonator driven by a coherent injected field
Gaussian aperture: FWHM=w
Injected field:wave vector=k
Mirror
Mirror
Acoskwf
Lf2i
f
Lf2C
kwf
LfL4Lf42i
f
LfL3Lf22B
kwf
LfL3Lf22i
f
L2fL4fDA
22
2
2
22
6422
2
322
22
322
2
22
L
L/2
Exact linear propagation taken into account by means of the ABCD matrix at the reference plane:
Instantaneous nonlinear medium located atthe reference plane
Small variation per cavity round trip TR of the adimensional field envelope E0(T,r) at the reference plane. Intracavity field carrier wave vector=k
NOTE: For f,w→∞ we get the Mean Field Limit equation considered for example in ref. M.Brambilla et al.,EPL 34, 1996 and in ref. W. J. Firth and A. J. Scroggie PRL 76, 1996
Diffusion Diffraction Space dependent gain|loss
Linear absorption
and dispersionSaturable
absorption <0
Injected field
inj020
002
02
020
R YE|E|1
E)i1(ErkCsin2
iReE
k
B
sin2
iImiE
k
B
sin2
iRe
T
ET
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Spontaneous emerging of intensity spots in the near field Parametric regime=-1, =-10.8, Yinj=6.52
Observation: In case (a) and (b) we managed to switch on and off a single intensity spot by superimposing a suitable addressing pulse to the holding beam !!
(a). Without Gaussian aperture (initial condition: null intracavity field+Gaussian distributed white noise)Time=9TR Time=23TR Time=541TR Time=280TR
(b). With Gaussian aperture (initial condition: null intracavity field+Gaussian distributed white noise)
Time=11TR Time=22TR Time=37TR Time=280TR
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WP 2
1Department of Physics, SUPA, University of Strathclyde, Glasgow, Scotland, UK2Institute of Physics, Academy of Sciences of Belarus, Minsk, Belarus
Y. Tanguy1, A. Smith, T. Ackemann,
F. Papoff, A. Scroggie, A. Yao1, W. J. Firth1
P. V. Paulau1,2, A. V. Naumenko2, N. A. Loiko2
VEGSEL with long cavity (task 2, overlap with WP1)
Planning and test setup for VCSEL + SA (task 1)
Modelling VEGSEL (task 2, overlap with WP1)
Modelling fast spatio-temporal dynamics with extended master equation (task 1, possibly 2)
Modelling coupled cavities (task 1, possibly 2)
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VEGSEL with long external cavity
actually setup from WP1 Yann showed (see also next slide)
• spot can be stationary (no peaks in RF- spectrum and FP)• spot can have weak sidemodes in FP• spectrum shows clearly strong excitation of sidemodes in FP
and peaks in RF spectrum (possibly due to background)• round-trip frequency 250 MHz
need for further analysis,
but potentially the spots would also qualify as CLB God knows how (ir)regular these might be
(simplified) model developed and coded from WP1 need to reintroduce carrier dynamics for reasonable results
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Spectra of spots
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Transfer to cavity light bullets
HR
HR
BSR 2-8%
self-imagingforward biased
lasera) reverse biased laser
(reduced reflectivity)b) QW SESAMc) QD SESAM
(reduced saturation fluence, no demagnification necessary)R0.8-0.985
R0.8-0.985
f18 mm
SAgain
possibilities:
f2100 mm
here: cut-off feedback to boundaries
f3200 mm
f45 mm
demagnification by factor of 3: adapt saturation fluences
set-up not yet tested, but could be done in week before Eastern, if considered to be necessary for annual report
R=0.8 about factor of eight in gain; R=0.9 about factor of four, R=0.985 ok
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Spectrum of SESAM
940 960 980 1000 1020 1040 10600.0
0.2
0.4
0.6
0.8
1.0
060323_SBR.opj
EPIC 2000532
R
wavelength (nm)
very high absorption losses, possibly not useful
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Extended Master equation
Dunlop et al., Opt. Lett. 21, 770 (1996)
ABCDnonlinearity
changeson time scale longer than round-trip time
changeson time scale of pulse
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Coupled cavities
coupling mirror between two Fabry-Perot cavities
transfer matrix
coupled master equations
only valid, if no variations on time-scale of round trip in both cavities (quasi single-longitudinal mode)
How to couple „extended“ master equations?
How to include inertia of medium?