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1APS-Sherwood Texas 2006-April 21-24
Study of nonlinear kinetic effects in Stimulated Raman
Scattering using semi-Lagrangian Vlasov codesAlain Ghizzo1, P. Bertrand1, T.W. Johnston2,
M. Albrecht-Marc1,T. Reveillé1
1. LPMIA, CNRS-UMR7040, Université Henri Poincaré, Nancy, BP 239, F-54506 Vandoeuvre, France
2. I.N.R.S. Energie et Matériaux, Varennes, Québec
2APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
3APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
4APS-Sherwood Texas 2006-April 21-24
Introduction
. Vlasov models have long been used to study collisionless plasmas.
• Vlasov codes: powerful tool for studying in details the particle dynamics due to very fine resolution in phase space.
Questions for applications:• Need for a kinetic model?• PIC or Vlasov simulation?
5APS-Sherwood Texas 2006-April 21-24
Vlasov plasmas: collective effects
A dichotomy experiment: (e,m) -> 2(e/2, m/2) -> 4(e/4, m/4) -> etc…
= dimensionless parameter, - divided by 2 at each dichotomy- « graininess parameter »
6APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
7APS-Sherwood Texas 2006-April 21-24
Comparison PIC-Vlasov (1)
Vlasov Codes
: real space dimension
is the graininess due to particules
PIC Codes
: momentum space dimension
: sampling of momentumspace in each direction
Sampling the x-space needs
Real space X momentum space
8APS-Sherwood Texas 2006-April 21-24
Comparison PIC-Vlasov (2)
Assume the same CPU time •to push a particle (PIC)•to move a phase space mesh point (Vlasov)
The ratio of the computationnal effort between Vlasov and PICdepends on•PIC graininess (must be as low as possible)•Sampling of momentum space (must be as high as possible)
9APS-Sherwood Texas 2006-April 21-24
Comparison PIC-Vlasov (3)
Dv =1 Dv =2 Dv =3
gPIC =10-2 1 100 10 000
gPIC =10-4 0.01 1 100
gPIC =10-6 0.0001 0.01 1
Prefer PIC
Prefer Vlasov
10APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
11APS-Sherwood Texas 2006-April 21-24
Stimulated Raman Scattering
Using Coulomb gauge
with
Vacuum PLASMA
Scattered wave (1)
Plasma wave (2)
LASER
Pump wave (0)
Vlasov equation for electrons 1D momentum space
12APS-Sherwood Texas 2006-April 21-24
SRS : 3 mode coupling
Vacuum PLASMA
Scattered wave (1)
Plasma wave (2)
LASER
Pump wave (0)
Quasi particles (photons, plasmons)
Energy conservation
Momentum conservation
Electron plasma in a fixed ion homogeneous background
€
ω0k0( )=ω1k1( )+ω2k2( )
€
k0=k1+k2
13APS-Sherwood Texas 2006-April 21-24
Three mode coupling : a fluid description
Scalar potential (Plasma mode)
Multiple time-space scale expansion of fluid equations
€
A⊥=12εA0(x
1,t1)ei(k0x0−ω0t0)+12εA1(x
1,t1)ei(k1x0−ω1t0)+c.c.
€
Ex(x,t)=12εE2x
1,t1( )eik2x0−ω2t0( )+c.c.
€
∂∂t=∂∂t0+ε
∂∂t1+L and
∂∂x=∂∂x0+ε
∂∂x1
Vector potential (electromagnetic modes)
14APS-Sherwood Texas 2006-April 21-24
Three mode coupling : a fluid description
Hydrodynamic equations for electronsAssume slowly varying envelopes: i.e.
with
€
∂∂t+vg0
∂∂x
⎛ ⎝ ⎜ ⎞
⎠ ⎟a0=−Γa1a2∂∂t+vg1
∂∂x
⎛ ⎝ ⎜ ⎞
⎠ ⎟a1=Γa2*a0∂∂t+vg2
∂∂x
⎛ ⎝ ⎜ ⎞
⎠ ⎟a2=Γa0a1*
€
Γ=e2mkωp
2ε0ω0ω1ω2( )1/2
15APS-Sherwood Texas 2006-April 21-24
Three mode coupling : a fluid description
Envelope equations + periodic conditions Action conservation
Energy density of mode i
Action density of mode i
photon (0) photon (1) plasmon (2)
€
S0+S1=const=C1S0+S2=const=C2
16APS-Sherwood Texas 2006-April 21-24
Time evolution: pump + scattered
Pump wave action
Scattered wave action
Goodconservation
Check the fluid predictions against a fully kinetic Vlasov simulation
17APS-Sherwood Texas 2006-April 21-24
Time evolution : pump + plasma
pump
plasma
Poor Conservation !
18APS-Sherwood Texas 2006-April 21-24
Phase space portraits (1)
Color scale
19APS-Sherwood Texas 2006-April 21-24
Phase space portraits (2)
Color scale
20APS-Sherwood Texas 2006-April 21-24
Phase space portraits (3)
Color scale
21APS-Sherwood Texas 2006-April 21-24
Accounting for « non fluid » particles
Good conservation
• Compute:Kinetic energy density above the lower separatrix:
• Divide by plasma wave frequency:
22APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
23APS-Sherwood Texas 2006-April 21-24
SRS-B in the « kinetic » regime (1)
• SRS-B reflectivity presents a bursting behavior
€
ω0=ωs+ωepw1 =2/3+1/3k0 = −ks+ kepw0.957=−0.60+1.559
• Nonlinear frequency shift - G.J. Morales and T.M. O’Neil, PRL 28, 417 (1972) -
24APS-Sherwood Texas 2006-April 21-24
SRS-B in the « kinetic » regime (2)
• Langmuir wave induced by SRS-B process
• Vortex-merging leading to weak turbulence
• BGK-like self-sustained structures (persisting over a long time)
25APS-Sherwood Texas 2006-April 21-24
Topics
1. Vlasov plasmas
2. Vlasov codes and PIC codes
3. Application I: Resonant wave particle interaction
4. Application II: SRS-B in optical mixing
5. Conclusions
26APS-Sherwood Texas 2006-April 21-24
Conclusions
Vlasov codes as compared to PIC codes
•lack of numerical noise •good resolution in phase space
provided the dimension of velocity space is as low as possible.
Kinetic effects in plasmas allow more phenomena than are found using only fluid theory with « ad hoc » kinetic damping.