Particle acceleration at shock waves moving at arbitrary speed: the case of large scale magnetic field and anisotropic scattering
arXiv:astro-ph/0701173 · doi:10.1086/512026
Abstract
A mathematical approach to investigate particle acceleration at shock waves moving at arbitrary speed in a medium with arbitrary scattering properties was first discussed in (Vietri 2003) and (Blasi & Vietri 2005}. We use this method and somewhat extend it in order to include the effect of a large scale magnetic field in the upstream plasma, with arbitrary orientation with respect to the direction of motion of the shock. We also use this approach to investigate the effects of anisotropic scattering on spectra and anisotropies of the distribution function of the accelerated particles.
28 pages, 14 figures, accepted for publication in ApJ
References in corpus (10)
- Particle acceleration by ultra-relativistic shocks: theory and simulations
- Particle acceleration at ultrarelativistic shocks: an eigenfunction method
- Energy spectra of cosmic rays accelerated at ultrarelativistic shock waves
- Ultra-high-energy cosmic ray acceleration by relativistic blast waves
- Particle acceleration and relativistic shocks
- Particle transport in tangled magnetic fields and Fermi acceleration at relativistic shocks
- Cosmic Ray Acceleration at Relativistic Shock Waves with a "Realistic" Magnetic Field Structure
- Relativistic Fermi acceleration with shock compressed turbulence
- On particle acceleration around shocks. I
- On particle acceleration around shocks II: a fully general method for arbitrary shock velocities and scattering media
Cited by in corpus (10)
- Diffusive Acceleration of Particles at Oblique, Relativistic, Magnetohydrodynamic Shocks
- A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays
- Kinetic simulations of mildly relativistic shocks I: particle acceleration in high Mach number shocks
- Kinetic Simulations of Cosmic-Ray-Modified Shocks I: Hydrodynamics
- New constraints on Planck-scale Lorentz Violation in QED from the Crab Nebula
- Interpretation and implication of the non-detection of GeV spectrum excess by Fermi gamma-ray Space Telescope in most GRBs
- Can we probe the Lorentz factor of gamma-ray bursts from GeV-TeV spectra integrated over internal shocks?
- The effect of energy amplification variance on the shock-acceleration
- Particle acceleration at shock waves: particle spectrum as a function of the equation of state of the shocked plasma
- Lepton Acceleration in Pulsar Wind Nebulae