Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Hig he r-o rde r Me tho ds fo r Simula ting L ig ht Pro pa g a tio - - PowerPoint PPT Presentation
Hig he r-o rde r Me tho ds fo r Simula ting L ig ht Pro pa g a tio - - PowerPoint PPT Presentation
Kur t Busch, Univer sit t Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de Hig he r-o rde r Me tho ds fo r Simula ting L ig ht Pro pa g a tio n a nd L ig ht-Ma tte r I nte ra c tio n in Na no -Pho to nic Syste ms K urt Busc h I
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Ac kno wle dg me nts
L a sha T ke she la shvili Mic ha e l K ö nig Je ns Nie g e ma nn Ja n Gie se le r Ma rtin Po to tsc hnig * K a i Sta nnig e l
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo tiva tio n
So lito n So lito n c o llisio n in a c o llisio n in a fib e r Bra g g g ra ting fib e r Bra g g g ra ting
L ine a r, no nline a r a nd q ua ntum o ptic a l pro b le ms in na no -pho to nic syste ms invo lve multiple time a nd le ng th sc a le s T his re q uire s a c c ura te , sta b le , a nd e ffic ie nt so lve rs fo r line a r a nd no nline a r Ma xwe ll’ s e q ua tio n a nd c o uple d syste ms
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo tiva tio n: Sta nda rd Appro a c he s
F DT D-Me tho d
Disc re tiza tio n o n Ye e -g rid 2nd o rde r in spa c e a nd time E ffic ie nt a nd e a sy to imple me nt
F inite -E le me nt-Me tho d
Disc re tiza tio n o n unstruc ture d g rids Hig he r-o rd e r in spa c e F re q ue nc y-d o ma in pre fe rre d
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo tiva tio n: Do no t trust Co mpute rs I
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo tiva tio n: Do no t trust Co mpute rs I I
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo tiva tio n: Do no t trust Co mpute rs I I I
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Silicon rods in air
Two-level atom (initially excited)
Mo tiva tio n: Do no t trust Co mpute rs I V
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Outline
T he K rylo v-Sub spa c e / Disc o ntinuo us Ga le rkin Appro a c h
– Ho w the me tho d wo rks a nd pe rfo rms – Adva nc e d spa tia l disc re tiza tio n
E xte nsio n to No nline a r & Co uple d Syste ms
– L a wso n-T ra nsfo rma tio n a nd Ro se nb ruc k-Wa nne r so lve rs – Pe rfo rma nc e
E xa mple s a nd Applic a tio ns
– Spo nta ne o us e missio n in pho to nic c rysta ls – Pla smo nic struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Outline
T he K rylo v-Sub spa c e / Disc o ntinuo us Ga le rkin Appro a c h
– Ho w the me tho d wo rks a nd pe rfo rms – Adva nc e d spa tia l disc re tiza tio n
E xte nsio n to No nline a r & Co uple d Syste ms
– L a wso n-T ra nsfo rma tio n a nd Ro se nb ruc k-Wa nne r so lve rs – Pe rfo rma nc e
E xa mple s a nd Applic a tio ns
– Spo nta ne o us e missio n in pho to nic c rysta ls – Pla smo nic struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
T he K rylo v-Sub spa c e Me tho d
Ma xwe ll e q ua tio ns in Sc hrö ding e r fo rm A fo rma l so lutio n o f is g ive n b y
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
T he K rylo v-Sub spa c e Me tho d
Disc re tiza tio n o f a nd (e .g . o n a Ye e -Grid )
- Ve ry la rg e b ut spa rse ma trix
Ma trix-Ve c to r-Pro d uc ts a re fe a sa b le We do no t re q uire the full ma trix , o nly its a c tio n
- n a ve c to r:
We do no t wa nt a ny re stric tio ns o n the pro pe rtie s
- f the ma trix (suc h a s ske w-symme try e tc .)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
T he K rylo v-Sub spa c e Me tho d
Build up the Krylov Subspa c e Ortho -no rma lize the b a sis b y Arno ldi-me tho d Ob ta in pro je c tio n o f o nto T he numb e r o f b a sis ve c to rs c a n b e sma ll (m~ 10)
- Ortho g o na l Ba sis
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
T he ke y a ppro xima tio n the n is Wo rks fo r a rb itra ry ma tric e s T he a c c ura c y o f the me tho d is a t le a st Me mo ry usa g e : (m+1)/ 2 re la tive to F DT D
T he K rylo v-Sub spa c e Me tho d
- J. Nie g e ma nn, L
. T ke she la shvili, a nd K . Busc h,
- J. Co mput. T
he o r. Na no sc i. 4, 627 (2007)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Co mpa riso n o f Pe rfo rma nc e (1D)
T he me tho d a llo ws muc h la rg e r time ste ps
FDTD Krylov (m=4) Krylov (m=8) Krylov (m=16) Krylov (m=32)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Co mpa riso n o f Pe rfo rma nc e (2D)
I n a 2D syste m, the e ffe c t is e ve n mo re pro no unc e d
FDTD K r y l
- v
( m = 4 ) Krylov (m=8) Krylov (m=16) K r y l
- v
( m = 3 2 )
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
I mpo rta nt Add -Ons - Via ADE s
Dispe rsive Ma te ria ls
– Drude -, L
- re ntz-, De b ye -Mo de l
– Se llma ie r-type Mo de ls
So urc e s Ope n Syste ms: Co mple x fre q ue nc y shifte d PML s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Ma te ria l Dispe rsio n via ADE s
All typic a l a na lytic dispe rsio n re la tio ns (Drude , L
- re ntz, De b ye ) c a n b e imple me nte d via ADE
s. E xpe rime nta l dispe rsio n fitte d b y c o mb ine d (multiple ) L
- re ntz- o r Drude -te rms.
E xa mple : (Sing le L
- re ntz-te rm)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Adva nc e d Spa tia l Disc re tiza tio n
With the K rylo v-sub spa c e me tho d , a c c ura c y o f time -inte g ra tio n c a n b e c hose n a rbitra rily Pro b le m: E rro r fro m the spa tia l disc re tiza tio n is limiting the to ta l a c c ura c y
- Hig he r o rde r ste nc ils
- Still o nly 2nd o rde r in the pre se nc e o f b o unda rie s
Po ssib le so lutio n: Ad a ptive g rid re fine me nt a ro und b o unda rie s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Unstruc ture d Grid in 1D
Ada pt the g rid so the po int de nsity is hig he r a ro und the ma te ria l b o unda rie s
n=1 n=1.5
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de FDTD Krylov (m=4) Krylov (m=8) Krylov (m=16) Krylov (m=32) Krylov (m=64) N=399 N=799 N=1599 N=3199
Unstruc ture d Grid Pe rfo rma nc e (1D)
4th-o rde r ste nc il a nd a da ptive g rids: 4th o rde r is ma inta ine d in the pre se nc e o f ma te ria l b o unda rie s
K . Busc h e t a l., physic a sta tus so lidi (b ) 244, 3479 (2007)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Unstruc ture d Grids in 2D/ 3D
Disc o ntinuo us Ga le rkin finite e le me nt te c hniq ue (b o rro we d fro m hydro dyna mic s)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Re sults o n Unstruc ture d Grids (2D)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Outline
T he K rylo v-Sub spa c e / Disc o ntinuo us Ga le rkin Appro a c h
– Ho w the me tho d wo rks a nd pe rfo rms – Adva nc e d spa tia l disc re tiza tio n
E xte nsio n to No nline a r & Co uple d Syste ms
– L a wso n-T ra nsfo rma tio n a nd Ro se nb ruc k-Wa nne r so lve rs – Pe rfo rma nc e
E xa mple s a nd Applic a tio ns
– Spo nta ne o us e missio n in pho to nic c rysta ls – Pla smo nic struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
E xte nsio n to No nline a r Syste ms
T he me tho d c a n b e e xte nde d to no nline a r syste ms L a wso n-T ra nsfo rma tio n:
- H is the line a r pa rt o f the no nline a r syste m
Ro se nb ruc k-Wa nne r so lve rs:
- H is the Ja c o b ia n o f the no nline a r syste m
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
E xte nsio n to No nline a r Syste ms
L a wso n-T ra nsfo rma tio n
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
E xte nsio n to No nline a r Syste ms
With a sta nda rd E ule r sc he me , o ne o b ta ins the “ L
a wson- E ule r Sc he me ”:
I n pra c tic e , we use a 4th-o rde r Rung e -K utta sc he me inste a d o f E ule r: “ L
a wson4”
Ro se nb ruc k-Wa nne r so lve r pro po se d b y Ho c hb ruc k a nd L ub ic h:“ Hoc hbruc k4”
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Pe rfo rma nc e Co mpa riso n
Dispe rsio n-fre e 1D syste m with K e rr-No nline a rity
F D T D L a wson4 Rung e -Kutta Hoc hbruc k4
- M. Po to tsc hnig e t a l., sub mitte d (2007)
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Outline
T he K rylo v-Sub spa c e / Disc o ntinuo us Ga le rkin Appro a c h
– Ho w the me tho d wo rks a nd pe rfo rms – Adva nc e d spa tia l disc re tiza tio n
E xte nsio n to No nline a r & Co uple d Syste ms
– L a wso n-T ra nsfo rma tio n a nd Ro se nb ruc k-Wa nne r so lve rs – Pe rfo rma nc e
E xa mple s a nd Applic a tio ns
– Spo nta ne o us e missio n in pho to nic c rysta ls – Pla smo nic struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Mo difie d Ra dia tio n Dyna mic s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Se mi-c la ssic a l De sc riptio n
F ull Ha milto nia n: F ie ld is tre a te d c la ssic a lly via Ma xwe ll’ s E q ua tio ns with po la riza tio n
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
I ntro duc ing the de nsity ma trix ρ whic h o b e ys
I nitia l po pula tio n diffe re nc e
T1: Relaxation T2: Dephasing γ : Dipole moment
Se mi-c la ssic a l De sc riptio n
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Se mi-c la ssic a l De sc riptio n
Ma xwe ll-Bo c h-E q ua tio ns in 1D
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Spo nta ne o us E missio n in 2D PhCs
- J. Nie g e ma nn e t a l., in pre pa ra tio n
Corresponding bandstructure Corresponding bandstructure
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Spo nta ne o us E missio n in 2D PhCs
- J. Nie g e ma nn e t a l., in pre pa ra tio n
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Spo nta ne o us E missio n in 2D PhCs
- J. Nie g e ma nn e t a l., in pre pa ra tio n
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Metallic cylinder (r=25nm, Ag) Gaussian pulse
Re so na nc e s o f Pla smo nic Struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Metallic cylinder (r=25nm, Ag) Gaussian pulse
Re so na nc e s o f Pla smo nic Struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Re so na nc e s o f Pla smo nic Struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Re so na nc e s o f Pla smo nic Struc ture s
Co urte sy o f Ma rtin Husnik
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
- M. Husnik e t a l., sub mitte d
Re so na nc e s o f Pla smo nic Struc ture s
Kur t Busch, Univer sit ät Kar lsr uhe, kur t @t fp.physik.uni-kar lsr uhe.de phot onics.t fp.uni-kar lsr uhe.de
Summa ry a nd Outlo o k
Hig he r-o rde r time -do ma in simula tio n o f the Ma xwe ll e q ua tio ns using K rylo v-sub spa c e me tho ds So urc e s, UPML s/ CPML a nd dispe rsive ma te ria ls (Se llme ie r-type ) via a uxilia ry fie lds Disc o ntino us Ga le rkin te c hniq ue fo r “c o nfo rma l” spa tia l disc re tiza tio n E xte nsio n to no nline a r a nd c o uple d syste ms’ dyna mic s F uture wo rk:
– Pa ra lle liza tio n –
Applic a tion to c omple x photonic syste ms