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Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma density electron density Solodov, C. Ren, J. Myatt, and R. Betti versity of Rochester oratory for Laser Energetics B. Mori, UCLA 3d Meeting of the Fusion Scien Center for Extreme States of Matt and Fast Ignition Physi University of Rochest 26–27 January 20

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Page 1: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density

Simulation of Plasma Wakefields and Weibel Instability of Electron Beams

in Plasma Using Codes LSP and OSIRIS

beam density plasma densityelectron density

A. Solodov, C. Ren, J. Myatt, and R. BettiUniversity of RochesterLaboratory for Laser EnergeticsW. B. Mori, UCLA

3d Meeting of the Fusion ScienceCenter for Extreme States of Matter

and Fast Ignition PhysicsUniversity of Rochester

26–27 January 2006

Page 2: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 3: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density

Codes LSP and OSIRIS

OSIRIS(developed at UCLA)

Explicit

PIC

LSP(product of MRC Albuquerque)

Explicit or Implicit

Particle (PIC) or Fluid

• Courant condition for the electromagnetic fields: Δt<Δx/c

• Numerical heating if Δx>3λD

• Courant condition is unnecessary in the implicit mode, non-resolved temporary modes are damped, remaining limitation: Δt < Δx/vte

• Implicit PIC: numerical heating or cooling if Δx>λD

• Implicit fluid: no numerical heating or cooling

Page 4: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 5: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 6: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 7: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 8: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 9: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 10: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 11: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 12: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 13: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 14: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 15: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 16: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density
Page 17: Simulation of Plasma Wakefields and Weibel Instability of Electron Beams in Plasma Using Codes LSP and OSIRIS beam density plasma densityelectron density

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