MHD-PIC Simulations of Cosmic-Ray Scattering and Transport in Inhomogeneously Ionized Plasma

Keyphrases

• Magnetohydrodynamics 100%
• Cosmic Rays 100%
• PIC Simulation 100%
• Scattering Rate 42%
• Alfvn Waves 28%
• Interstellar Medium 28%
• Spatial Gradient 28%
• Pressure Gradient 14%
• First-principles 14%
• Molecular Gas 14%
• Mean Free Path 14%
• Quasi-linear 14%
• Periodic Domain 14%
• High Density 14%
• Wave Scattering 14%
• Cosmic Background 14%
• Fokker-Planck 14%
• Transport Coefficients 14%
• Kinetic Physics 14%
• Distribution Function 14%
• Neutral Drag 14%
• Chemical Composition 14%
• Translational Symmetry 14%
• Dynamical Motion 14%
• Self-generated 14%
• Energetic Particles 14%
• Pitch Angle Scattering 14%
• Atomic Gases 14%
• Transport Problem 14%
• Cosmic Ray Flux 14%
• Ionization State 14%
• Background Gas 14%
• Wave-particle 14%
• Particle Scattering 14%
• Low-density Plasma 14%
• Damping Region 14%
• Critical Impact 14%
• Cosmic Ray Transport 14%
• Ray Distribution 14%
• Cosmic Ray Propagation 14%
• Particle Stream 14%
• Hydrodynamic Formulation 14%
• Reduced Scattering 14%
• Comprehensive Calibration 14%
• Simulation Domain 14%
• Particle-in-cell Simulation 14%
• Flux-form 14%

Physics

• Magnetohydrodynamics 100%
• Plasma Physics 100%
• Transportation 100%
• Interstellar Matter 66%
• Hydrodynamics 66%
• Pressure Gradient 33%
• Physics 33%
• Distribution Function 33%
• Energetic Particle 33%
• Mean Free Path 33%
• First Principle 33%
• Transport Property 33%
• Molecular Gas 33%
• Monatomic Gas 33%
• Wave Scattering 33%
• Plasma Density 33%
• Translational Symmetry 33%