Diffusive Shock Acceleration with Magnetic Amplification by Non-resonant Streaming Instability in SNRs

Abstract

We investigate the diffusive shock acceleration in the presence of the non-resonant streaming instability introduced by Bell (2004). The numerical MHD simulations of the magnetic field amplification combined with the analytical treatment of cosmic ray acceleration permit us to calculate the maximum energy of particles accelerated by high-velocity supernova shocks. The estimates for Cas A, Kepler, SN1006, and Tycho historical supernova remnants are given. We also found that the amplified magnetic field is preferentially oriented perpendicular to the shock front downstream of the fast shock. This explains the origin of the radial magnetic fields observed in young supernova remnants.

18 pages, 9 figures, accepted to ApJ

References in corpus (16)

• Simulations of small-scale turbulent dynamo
• On the magnetic fields and particle acceleration in Cas A
• Magnetic Field Amplification in Tycho and other Shell-type Supernova Remnants
• Fine Structures of Shock of SN 1006 with the Chandra Observation
• Young core collapse supernova remnants and their supernovae
• On the spectrum of high-energy cosmic rays produced by supernova remnants in the presence of strong cosmic-ray streaming instability and wave dissipation
• On the role of injection in kinetic approaches to nonlinear particle acceleration at non-relativistic shock waves
• PSR J2229+6114: Discovery of an Energetic Young Pulsar in the Error Box of the EGRET Source 3EG J2227+6122
• Emission of SN 1006 produced by accelerated cosmic rays
• The theory of synchrotron emission from supernova remnants
• Modeling Bell's Non-resonant Cosmic Ray Instability
• Chandra Observations of A Galactic Supernova Remnant Vela Jr.: A New Sample of Thin Filaments Emitting Synchrotron X-Rays
• Variation of cosmic ray injection across supernova shocks
• Turbulence and particle acceleration in collisionless supernovae remnant shocks: I-Anisotropic spectra solutions
• The Evolution of Adiabatic Supernova Remnants in a Turbulent, Magnetized Medium
• Induced Scattering and Two-Photon Absorption of Alfven Waves with Arbitrary Propagation Angles

Cited by in corpus (104)

• Cosmic ray acceleration and escape from supernova remnants
• The microphysics of collisionless shock waves
• The 1st Fermi Lat Supernova Remnant Catalog
• The origin of Galactic cosmic rays: challenges to the standard paradigm
• A kinetic approach to cosmic ray induced streaming instability at supernova shocks
• Nonthermal Radiation of Young Supernova Remnants
• Spectrum of Galactic Cosmic Rays Accelerated in Supernova Remnants
• Observational signatures of particle acceleration in supernova remnants
• Non-linear Study of Bell's Cosmic Ray Current-driven Instability
• Cosmic Ray Transport in the Galaxy: a Review
• Efficient cosmic ray acceleration, hydrodynamics, and Self-consistent Thermal X-ray Emission applied to SNR RX J1713.7-3946
• Diffusive shock acceleration and magnetic field amplification
• Analytic Solution for Self-regulated Collective Escape of Cosmic Rays from their Acceleration Sites
• Magnetic Field Amplification in Galaxy Clusters and its Simulation
• Dynamical Feedback of Self-generated Magnetic Fields in Cosmic Ray Modified Shocks
• Escaping the accelerator; how, when and in what numbers do cosmic rays get out of supernova remnants?
• Spectra of Cosmic Ray Protons and Helium Produced in Supernova Remnants
• Cosmic ray acceleration in young supernova remnants
• Cosmic ray acceleration at oblique shocks
• Origin of Cosmic Rays
• Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
• Universal behaviour of shock precursors in the presence of efficient cosmic-ray acceleration
• Microphysics of cosmic ray driven plasma instabilities
• Particle acceleration in astrophysical jets
• High-energy particles and radiation in star-forming regions
• Cosmic-ray current driven turbulence in shocks with efficient particle acceleration: the oblique, long-wavelength mode instability
• Core-collapse model of broadband emission from SNR RX J1713.7-3946 with thermal X-rays and Gamma-rays from escaping cosmic rays
• Supernova Remnants Interacting with Molecular Clouds: X-ray and Gamma-ray Signatures
• Type IIn supernovae as sources of high energy astrophysical neutrinos
• A filamentation instability for streaming cosmic-rays
• Two-Dimensional particle-in-cell simulations of the nonresonant, cosmic-ray driven instability in SNR shocks
• Numerical simulations of diffusive shock acceleration in SNRs
• A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant
• Gamma-ray emission of accelerated particles escaping a supernova remnant in a molecular cloud
• Particle acceleration by shocks in supernova remnants
• Plasma instabilities as a result of charge exchange in the downstream region of supernova remnant shocks
• Core collapse supernovae as Cosmic Ray sources
• Particle Spectra from Acceleration at Forward and Reverse Shocks of Young Type Ia Supernova Remnants
• Internal dynamics and particle acceleration in Tycho's SNR
• A Model of Polarized X-ray Emission from Twinkling Synchrotron Supernova Shells
• Postshock turbulence and diffusive shock acceleration in young supernova remnants
• Cosmic rays in galactic and extragalactic magnetic fields
• Steady-State Solutions in Nonlinear Diffusive Shock Acceleration
• Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy
• Magnetic fields in cosmic particle acceleration sources
• Time-Dependent Escape of Cosmic Rays from Supernova Remnants, and their Interaction with Dense Media
• Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
• Nonthermal radiation of young supernova remnants: the case of Cas A
• X-ray polarization detection of Cassiopeia A with IXPE
• Faraday Rotation Measure Variations of Repeating Fast Radio Burst Sources
• Spectra of magnetic fluctuations and relativistic particles produced by a nonresonant wave instability in supernova remnant shocks
• Synchrotron Emission from Elliptical Galaxies Consequent to AGN outbursts
• A young SNR illuminating nearby Molecular Clouds with cosmic rays
• Tracing the sources of cosmic rays with molecular ions
• Non-Maxwellian Proton Velocity Distributions in Nonradiative Shocks
• On physical and numerical instabilities arising in simulations of non-stationary radiatively cooling shocks
• X-ray polarimetry reveals the magnetic field topology on sub-parsec scales in Tycho's supernova remnant
• Theory of cosmic ray and gamma-ray production in the supernova remnant RX J0852.0-4622
• Cosmic-ray-induced ionization in molecular clouds adjacent to supernova remnants - Tracing the hadronic origin of GeV gamma radiation
• Leaked GeV CRs from a broken shell: Explaining 9 years Fermi-LAT data of SNR W28
• When disorder looks like order: a new model to explain radial magnetic fields in young supernova remnants
• Amplification of perpendicular and parallel magnetic fields by cosmic ray currents
• H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A
• Cosmic Ray Origins in Supernova Blast Waves
• 3-D Model of Broadband Emission from Supernova Remnants Undergoing Non-linear Diffusive Shock Acceleration
• Nonthermal Radiation from Supernova Remnants: Effects of Magnetic Field Amplification and Particle Escape
• 3D Simulations of the Thermal X-ray Emission from Young Supernova Remnants Including Efficient Particle Acceleration
• 3D simulations of the non-thermal broad-band emission from young supernova remnants including efficient particle acceleration
• Particle acceleration and magnetic field amplification in massive young stellar object jets
• Aperiodic magnetic turbulence produced by relativistic ion beams
• Three-dimensional simulations of non-resonant streaming instability and particle acceleration near non-relativistic astrophysical shocks
• On the background-gyroresonant character of the Bell instability
• Diffusive shock acceleration with magnetic field amplification and Alfvenic drift
• Radio polarimetry signatures of strong magnetic turbulence in Supernova Remnants
• Lepton-driven Non-resonant Streaming Instability
• Effects of Alfvenic Drift on Diffusive Shock Acceleration at Weak Cluster Shocks
• Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array
• Time Variability of Nonthermal X-ray Stripes in Tycho's Supernova Remnant with Chandra
• Cosmic Ray Acceleration in Hydromagnetic Flux Tubes
• Evolution of Magnetic Fields and Cosmic Ray Acceleration in Supernova Remnants
• Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array
• Radioactivity and Electron Acceleration in Supernova Remnants
• A Spatially Resolved Study of X-ray Properties in Superbubble 30 Dor C with $XMM-Newton$
• Practical aspects of X-ray imaging polarimetry of supernova remnants and other extended sources
• Stochastic re-acceleration and magnetic-field damping in Tycho's supernova remnant
• Cosmic-ray current-driven instabilities -- revisiting environmental conditions
• X-ray polarization: A view deep inside cosmic ray driven turbulence and particle acceleration in supernova remnants
• Ultra high energy cosmic rays from past activity of Andromeda galaxy
• Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
• Is the SNR HESS J1731-347 colliding with molecular clouds?
• Origin of Spectral Hardening of Secondary Cosmic-Ray Nuclei
• Cosmic ray transport and acceleration with magnetic mirroring
• Escape of cosmic rays from perpendicular shocks in the circumstellar magnetic field
• The TeV supernova remnant shell HESS J1731-347 and its surroundings
• Spatially decomposed $\gamma$-ray features surrounding SNR Kes 79 & PSR J1853+0056
• HESS J1858+020: A GeV-TeV source possibly powered by CRs from SNR G35.6-0.4
• Acceleration of Heavy Ions at Non-Relativistic Collisionless Shocks
• SNR G54.1+0.3, a PeVatron candidate unveiled by LHAASO
• PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433
• Structure of a strong supernova shock wave and rapid electron acceleration confined in its transition region
• An Asymmetrical Model for High Energy Radiation of Cassiopeia A
• Role of the radiative stage for cosmic ray acceleration in SNRs
• Can superbubbles accelerate ultra-high energy protons?
• Escape of cosmic rays from perpendicular shocks in the interstellar magnetic field