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Transcript of otws2_7351
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Stochastic Maxwell Equations in Photonic CrystalModeling and Simulations
Hao-Min Zhou
School of Math, Georgia Institute of Technology
Joint work with:
Ali Adibi (ECE), Majid Badiei (ECE), Shui-Nee Chow (Math)
IPAM, UCLA, April 14-18, 2008
Partially supported by NSF
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Outline
Introduction & Motivation
Direct Method A Stochastic Model
Wiener Chaos Expansions (WCE) Numerical Method based on WCE
Simulation results Conclusion
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Introduction & Motivation
Stochastic PDEs :
Solutions are no longer deterministic.
Main interest: statistical properties, suchas mean, variance.
Multi-scale structures.
Fluid DynamicsEngineering
Material Sciences
Biology
Finance
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Introduction & Motivation
),(),(),( tyytyJtyJ jiji = Spatially incoherent source:
),( tyJ j
),( tyJ i
Such as diffuse light in optics.
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Introduction & Motivation
Applications in sensing
Raman spectroscopy for bio and environmental sensing
Photonic Crystal
spectrometer(in nano-scale)
Humantissue
Spatially incoherent
light
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Photonic Crystal Spectrometer
IncidentSpatially IncoherentField
Detectors
Output A
Output B
Output C
Output D
Output E
Output F
HeterogeneousPhotonic Structure
SpectrallyDiverseField
Multiplex multimodal spectrometer
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Introduction & Motivation
Photonic Crystal (designed) as the medium
goal: model the incoherent source and simulate output
First step in the design of Photonic Crystal spectrometers
Wave propagation is governed by Maxwell equations
a
Input Source(incoherent)
at A
Output at B(electric field
intensity)
),( tyJ ),( tyE2
Optimal design of the shapes of Photonic Crystals for largest band gap (Kao-
Osher-Yablonovitch, 05)
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Maxwell Equation
Maxwell equations:
ttt
= ),(),( rHrE
),(),(
)(),( tt
tt rJ
rErrH +
=
0= E
0= H
t
t
t
tt
=
),(),()(),(
2
2rJrE
rrE
Helmholtz wave equation:
electric field
magnetic field
Input incoherent source)J(r,t
)E(r,t)H(r,t
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Helmholtz wave equation
z-invariant structure implies
two sets of decoupled equations Transverse Magnetic (TM) (Ez,Hx,Hy)
Transverse Electric (TE) (Hz,Ex,Ey)
3D space structure reduces to 2D
Helmholtz TM wave equation:
tttyyxx tyxJtyxEyxtyxEtyxE )),,(()),,()(,()),,(()),,(( =+
PDEs are linear.
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Direct Method for PC Spectrometer
Incoherent property implies the direct (brute-force) method.
Input nonzero point source at , and
Compute output electric field at B
Total electric intensity at B:
Why point source? Non-point sources, such as plane waves,lead to coherent outputs.
Pro: correct physics (linear equations + incoherent outputs).
Con: very inefficient.
),( tyJi
piy
).(,0),( ijtyJ jp =
2 2( , , ) ( ( , , )) .pB i Bi
E x y t E x y t=
),( tyEpi
+=ji
p
j
p
i
i
p
i
i
p
i EEEE,
22 )()(
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A Stochastic Model
Spatially incoherent source
Stochastic model
More general:
tttyyxx tyxJtyxEyxtyxEtyxE )),,(()),,()(,()),,(()),,(( =+
)()(),,( tVyXtyxJ Az =
?
( )
=
2
0
0 exp)(sin)(T
tttttV
10ax10a Photonic Crystal asthe simulation medium
a
),()( ydWyX = )(yW Brownian Motion.
( , , ) ( , , ) ( , , ),tJ x y t f x y t dW x y t=
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Stochastic Helmholtz Wave Equations
Current density is a stochastic source.
Solution for electric field is random.
Monte Carlo simulation is slow, and hard to recover the
incoherent properties
Our strategy: WCE.
tttyyxx tyxJtyxEyxtyxEtyxE )),,(()),,()(,()),,(()),,(( =+
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Monte Carlo
Traditional methods, Monte Carlo (MC)
simulations,
Not many computational methods available.
Solve the equations realization by realization.
Each realization, the equations become deterministic and
solved by classical methods.The solutions are treated as samples to extract statistical
properties.
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Monte Carlo
MC can be very expensive:
Has slow convergence, governed by law of large numbers
and the convergence is not monotone.( is the number ofMC realizations)
Need to resolve the fine scales in each realization to obtainthe small scale effects on large scales, while only large scale
statistics are of interests, such as long time and large scale
behaviors.
Hard to estimate errors
Must involve random number generators, which need to be
carefully chosen.
),1
(
n
O
n
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Wiener Chaos Expansions
Goal: Design efficient numerical methods.
Separate the deterministic properties from
randomness.
Has better control on the errors.
Avoid random number generators, all
computations are deterministic.
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Wiener Chaos Expansions
Functions depends on Brownian
motion
),,( dWxtu
.W
contains infinitely many independent
Gaussian random variables, is time and/or spatialdependent.
WCE: decompose by orthogonalpolynomials, similar to a spectral method, but
for random variables.
),,( dWxtu
W
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Wiener Chaos Expansions
any orthonormal basis of , such
as harmonic functions in our computations.
)(smi ),0(2
YL
Define which are independent
Gaussian.
,)(0
=Y
sii dWsm
Let construct Wicks products),,,( 21 =
=
=1
).()(i
iiHT
is a multi-index, Hermite polynomials.)( iiH
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Wiener Chaos Expansions
Cameron-Martin(1947): any
can be decomposed as
),,( dWxtu
= ),(),(),,( aTxtudWxtu
where
)).(),,((),( TxtuExtu =
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Wiener Chaos Expansions
Statistics can be reconstructed from Wiener
Chaos coefficientsmean ),,(),( 0 xtuxtEu =
variance
22 ),)(( =
uxtuE
Higher order moments can be computed too.
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Wiener Chaos Expansions
Properties of Wicks products:
,1))(( 0 =TE
0,0))(( = TE
= 1
0
)( TTE
=
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Wiener Chaos Expansions
Wiener Chaos expansions have been
used in
Nonlinear filtering, Zakai equation (Lototsky, Mikulevicius
& Rozovskii, 97)
Stochastic media problems (Matthies & Bucher, 99)
Theoretical study of Stochastic Navier-Stokes equations
(Mikulevicius & Rozovskii, 02)
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Hermite Polynomial Expansions
A long history of using Hermite polynomials in
PDEs containing Gaussian random variables.
Random flows: Orszag & Bissonnette (67),Crow & Canavan (70),
Chorin (71,74),Maltz & Hitzl (79),
Stochastic finite element: Ghanem, et al (91,99, ).
Spectral polynomial chaos expansions:Karniadakis, Su and collaborators (a collection of papers), and
WCE for problems in fluid: Hou, Rozovskii, Luo, Zhou (04)
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WCE for stochastic Helmholtz equation
Expand the source and electric field:
Take advantage of
Equation is linear, so electric field hasexpansion
)(),(),,( ii
TtyJdWtyJ
=
=
=1
)()(i
ii ymydW
)(),,(),,,( ii TtyxEdWtyxE =
= ii ymtVdWtyJ )()(),,( Only Gaussian (linear)
= ii tyxEdWtyxE ),,(),,,(
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WCE for stochastic Helmholtz equation
The stochastic equation is converted into a
collection (decoupled) of deterministic
Helmholtz equations
Standard numerical methods, such as finite
difference time domain (FDTD) in oursimulation, can be applied.
)())(()),,()(,()),,(()),,(( ymtVtyxEyxtyxEtyxE itttiyyixxi =+
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WCE for stochastic Helmholtz equation
The electric fields from point sources
can be recovered by
Other moments can be computed by point
source solutions in the standard ways.
Under relative general conditions, WCE
coefficients decay quickly,
),,( tyxEpi
=j
jij
p
i tyxEymtyxE ),,()(),,(
1,
i r
E Oi
r Related to the smoothnessof the solutions.
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Simulation of a spatially incoherent source
Extremely fast convergence for 10ax10a example
Comparison of the direct method
(brute-force) simulation and the
WCE method
Convergence of the WCE method
S l f ll h
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Simulation of a spatially incoherent source (3)
Less than 1% error and more than one order of magnitude faster simulation,
Over 2 order of magnitude faster simulations for practical photonic crystals.
For 15 coefficients the gain in simulation time is 32, i.e., 32 times faster simulation
Percentage
error
Number of coefficients
20ax10a
For a 20ax10a example (doubled sized)
C l i
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Conclusion
Proposed a stochastic model for incoherent source
Design a fast numerical method based on WCE to
simulate the incoherent source for photonic crystals.
The method can be coupled with other fast Maxwell
equations solvers.
More than 2 order of magnitude faster simulations can
be achieved for practical structures.
The model and method are general and can be applied
to other types of stochastic problems involving incoherent
sources.