On the role of injection in kinetic approaches to nonlinear particle acceleration at non-relativistic shock waves
arXiv:astro-ph/0505351 · doi:10.1111/j.1365-2966.2005.09227.x
Abstract
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi process can be determined within kinetic models that account for both the hydrodynamics of the shocked fluid and the transport of the accelerated particles. These models predict the appearance of multiple solutions, all physically allowed. We discuss here the role of injection in selecting the real solution, in the framework of a simple phenomenological recipe, which is a variation of what is sometimes referred to as thermal leakage. In this context we show that multiple solutions basically disappear and when they are present they are limited to rather peculiar values of the parameters. We also provide a quantitative calculation of the efficiency of particle acceleration at cosmic ray modified shocks and we identify the fraction of energy which is advected downstream and that of particles escaping the system from upstream infinity at the maximum momentum. The consequences of efficient particle acceleration for shock heating are also discussed.
References in corpus (12)
- Limits on diffusive shock acceleration in supernova remnants in the presence of cosmic-ray streaming instability and wave dissipation
- Acceleration Rates and Injection Efficiencies in Oblique Shocks
- A semi-analytical approach to non-linear shock acceleration
- Analytic solution for nonlinear shock acceleration in the Bohm limit
- Non-linear Particle Acceleration in Oblique Shocks
- Numerical Studies of Cosmic Ray Injection and Acceleration
- Ion leakage from quasiparallel collisionless shocks: implications for injection and shock dissipation
- Non-linear shock acceleration in the presence of seed particles
- Efficiency of Nonlinear Particle Acceleration at Cosmic Structure Shocks
- Critical self-organization of astrophysical shocks
- Diffusive Shock Acceleration Simulations: Comparison with Particle Methods and Bow Shock Measurements
- Diffusive Shock Acceleration in Oblique MHD Shocks: Comparison with Monte Carlo Methods and Observations
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- Diffuse Hard X-ray Emission in Starburst Galaxies as Synchrotron from Very High Energy Electrons
- The Supernova Remnant W44: confirmations and challenges for cosmic-ray acceleration
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- Spectra of accelerated particles at supernova shocks in the presence of neutral hydrogen: the case of Tycho
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