The maximum momentum of particles accelerated at cosmic ray modified shocks
arXiv:astro-ph/0612424 · doi:10.1111/j.1365-2966.2006.11412.x
Abstract
Particle acceleration at non-relativistic shocks can be very efficient, leading to the appearance of non-linear effects due to the dynamical reaction of the accelerated particles on the shock structure and to the non-linear amplification of the magnetic field in the shock vicinity. The value of the maximum momentum in these circumstances cannot be estimated using the classical results obtained within the framework of test particle approaches. We provide here the first attempt at estimating in the cosmic ray modified regime, taking into account the non-linear effects mentioned above.
arXiv comment15 Pages, 2 figures, MNRAS in press
References in corpus (13)
- Cosmic Ray Acceleration at the Forward Shock in Tycho's Supernova Remnant: Evidence from Chandra X-ray Observations
- On the role of injection in kinetic approaches to nonlinear particle acceleration at non-relativistic shock waves
- 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
- Nonlinear Diffusive Shock Acceleration with Magnetic Field Amplification
- A general solution to non-linear particle acceleration at non-relativistic shock waves
- Non-linear Particle Acceleration in Oblique Shocks
- Numerical Studies of Cosmic Ray Injection and Acceleration
- 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 in Oblique MHD Shocks: Comparison with Monte Carlo Methods and Observations
Cited by in corpus (72)
- Design Concepts for the Cherenkov Telescope Array
- The Origin of Galactic Cosmic Rays
- Broad-band nonthermal emission from molecular clouds illuminated by cosmic rays from nearby supernova remnants
- Strong evidences of hadron acceleration in Tycho's Supernova Remnant
- The 1st Fermi Lat Supernova Remnant Catalog
- Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. II: anisotropy
- Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. I: spectrum and chemical composition
- Rise and Fall of Radio Halos in Simulated Merging Galaxy Clusters
- The origin of galactic cosmic rays
- Searching for galactic cosmic ray pevatrons with multi-TeV gamma rays and neutrinos
- Dynamical Feedback of Self-generated Magnetic Fields in Cosmic Ray Modified Shocks
- Gamma ray emission from SNR RX J1713.7-3946 and the origin of galactic cosmic rays
- Cosmic-ray acceleration in supernova remnants: non-linear theory revised
- Simulations of Ion Acceleration at Non-relativistic Shocks. III. Particle Diffusion
- Particle Acceleration in Supernova Remnants and the Production of Thermal and Nonthermal Radiation
- Antiprotons from dark matter annihilation in the Galaxy: astrophysical uncertainties
- On the escape of particles from cosmic ray modified shocks
- Space- and Ground-Based Gamma-Ray Astrophysics
- Cosmic-ray-induced filamentation instability in collisionless shocks
- Particle acceleration in astrophysical jets
- Non-linear diffusive shock acceleration with free escape boundary
- Magnetic field amplification in nonlinear diffusive shock acceleration including resonant and non-resonant cosmic-ray driven instabilities
- Cosmic-ray current driven turbulence in shocks with efficient particle acceleration: the oblique, long-wavelength mode instability
- Kinetic Simulations of Cosmic-Ray-Modified Shocks II: Particle Spectra
- Dynamical effects of self-generated magnetic fields in cosmic ray modified shocks
- "Espresso" Acceleration of Ultra-high-energy Cosmic Rays
- Spatial structure of X-ray filaments in SN 1006
- Self-Similar Evolution of Cosmic-Ray-Modified Quasi-Parallel Plane Shocks
- Non-linear diffusive acceleration of heavy nuclei in supernova remnant shocks
- A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant
- Supernova Remnants in the Local Group I: A model for the radio luminosity function and visibility times of supernova remnants
- Contribution of starburst nuclei to the diffuse gamma-ray and neutrino flux
- Radio Halos From Simulations And Hadronic Models I: The Coma cluster
- Comparison of Different Methods for Nonlinear Diffusive Shock Acceleration
- Shock acceleration of electrons in the presence of synchrotron losses: I. test particle theory
- Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
- Signatures of the transition from galactic to extragalactic cosmic rays
- X-ray Stripes in Tycho's Supernova Remant: Synchrotron Footprints of a Nonlinear Cosmic Ray-driven Instability
- Steady-State Solutions in Nonlinear Diffusive Shock Acceleration
- Collisionless shocks in a partially ionized medium: III. Efficient cosmic ray acceleration
- Understanding hadronic gamma-ray emission from supernova remnants
- Time-dependent particle acceleration in supernova remnants in different environments
- dHybridR: a Hybrid--Particle-in-Cell Code Including Relativistic Ion Dynamics
- A cosmic-ray precursor model for a Balmer-dominated shock in Tycho's supernova remnant
- Bottom-up Acceleration of Ultra-High-Energy Cosmic Rays in the Jets of Active Galactic Nuclei
- Steep Cosmic Ray Spectra with Revised Diffusive Shock Acceleration
- Magnetic Field Amplification and Rapid Time Variations in SNR RX J1713.7-3946
- 3-D Model of Broadband Emission from Supernova Remnants Undergoing Non-linear Diffusive Shock Acceleration
- Espresso and Stochastic Acceleration of Ultra-high-energy Cosmic Rays in Relativistic Jets
- Particle acceleration and non-thermal emission in colliding-wind binary systems
- UHE neutrinos from Pop III stars: concept and constraints
- Diffuse Galactic Gamma Rays at intermediate and high latitudes. I. Constraints on the ISM properties
- Lack of thermal energy in superbubbles: hint of cosmic rays?
- The multi-band nonthermal emission from the supernova remnant RX J1713.7-3946
- Gamma Rays and Neutrinos from SNR RX J1713.7-3946
- Non-linear diffusive shock acceleration: A recipe for injection of electrons
- Kinetic approaches to particle acceleration at cosmic ray modified shocks
- Hybrid Simulations of Particle Acceleration at Shocks
- Hydrodynamical and radio evolution of young supernova remnant G1.9+0.3 based on the model of diffusive shock acceleration
- Origin of Galactic Cosmic Rays
- Hadronic versus leptonic origin of gamma-ray emission from supernova remnants
- Time-dependent shock acceleration of particles. Effect of the time-dependent injection, with application to supernova remnants
- The role of ionization in the shock acceleration theory
- Particle acceleration in interstellar shocks
- Direct Measurements, Acceleration and Propagation of Cosmic Rays
- Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae
- Non-linear Diffusive Shock Acceleration of Cosmic Rays -- Quasi-thermal and Non-thermal Particle Distributions
- Modelling Giant Radio Halos
- On the Gamma Ray Burst Origin of Extremely Energetic Cosmic Rays
- New insights on hadron acceleration at supernova remnant shocks
- Espresso Acceleration of Ultra-High-Energy Cosmic Rays up to the Hillas Limit in Relativistic MHD Jets
- Theory of nonlinear particle acceleration at shocks and self-generation of the magnetic field