Limits on diffusive shock acceleration in supernova remnants in the presence of cosmic-ray streaming instability and wave dissipation

Abstract

The instability in the cosmic-ray precursor of a supernova shock moving in interstellar medium is studied. The level of magnetohydrodynamic turbulence in this region determines the maximum energy of particles accelerated by the diffusive shock acceleration mechanism. The high efficiency of cosmic ray acceleration is accepted, and the consideration is not limited by the case of weak turbulence. It is assumed that Kolmogorov type nonlinear wave interactions together with the ion-neutral collisions restrict the amplitude of random magnetic field. As a result, the maximum energy of accelerated particles strongly depends on the age of supernova remnant. The maximum energy can be as high as $\sim 10^{17}Z$ eV in young supernova remnants and falls down to about $\sim 10^{10}Z$ eV at the end of Sedov stage. Thus the standard estimate of maximum particle energy based on the Bohm limit calculated for the interstellar magnetic field strength is not justified in this case. This finding may explain why the supernova remnants with the age more than a few thousand years are not prominent sources of very high energy gamma-rays.

10 pages, 2 figures

Cited by in corpus (110)

• Fast variability of TeV gamma-rays from the radio galaxy M 87
• Cosmic ray acceleration and escape from supernova remnants
• The Milky Way's Kiloparsec Scale Wind: A Hybrid Cosmic-Ray and Thermally Driven Outflow
• Strong evidences of hadron acceleration in Tycho's Supernova Remnant
• The microphysics of collisionless shock waves
• Cosmic Ray Scattering and Streaming in Compressible Magnetohydrodynamic Turbulence
• Spectral breaks as a signature of cosmic ray induced turbulence in the Galaxy
• The 1st Fermi Lat Supernova Remnant Catalog
• Fermi-LAT Discovery of Extended Gamma-ray Emission in the Direction of Supernova Remnant W51C
• Observational constraints on energetic particle diffusion in young SNRs: amplified magnetic field and maximum energy
• On the spectrum of high-energy cosmic rays produced by supernova remnants in the presence of strong cosmic-ray streaming instability and wave dissipation
• Superbubbles and Energetic Particles in the Galaxy. I: Collective effects of particle acceleration
• On the role of injection in kinetic approaches to nonlinear particle acceleration at non-relativistic shock waves
• Detection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II
• Spectrum of Galactic Cosmic Rays Accelerated in Supernova Remnants
• Cosmic Ray Transport in the Galaxy: a Review
• Spectrum of cosmic rays, produced in supernova remnants
• Evolution of the cosmic ray anisotropy above 10^{14} eV
• Escape-limited Model of Cosmic-ray Acceleration Revisited
• Nonlinear Diffusive Shock Acceleration with Magnetic Field Amplification
• The contribution of supernova remnants to the galactic cosmic ray spectrum
• The theory of synchrotron emission from supernova remnants
• Modeling Bell's Non-resonant Cosmic Ray Instability
• Non-linear shock acceleration in the presence of seed particles
• Cosmic ray driven Galactic winds
• Numerical Studies of Diffusive Shock Acceleration at Spherical Shocks
• Propagation of galactic cosmic rays in the presence of self-generated turbulence
• Spectrum and Anisotropy of Cosmic Rays at TeV-PeV-energies and Contribution of Nearby Sources
• Grammage of cosmic rays around Galactic supernova remnants
• Nonlinear Particle Acceleration at Reverse Shocks in Supernova Remnants
• On the radial distribution of Galactic cosmic rays
• Escape of cosmic-ray electrons from supernova remnants
• Exploring particle escape in supernova remnants through gamma rays
• Recombining Plasma and Hard X-ray Filament in the Mixed-Morphology Supernova Remnant W44
• Detailed Investigation of the Gamma-Ray Emission in the Vicinity of SNR W28 with FERMI-LAT
• The Origin of Galactic Cosmic Rays as Revealed by their Composition
• Supernova remnants in clumpy media: particle propagation and gamma-ray emission
• The supernova remnant W44: a case of cosmic-Ray reacceleration
• Self-Generated Cosmic-Ray Turbulence Can Explain the Morphology of TeV Halos
• Internal dynamics and particle acceleration in Tycho's SNR
• High Energy Gamma-Ray Astronomy
• Postshock turbulence and diffusive shock acceleration in young supernova remnants
• Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy
• Turbulence and particle acceleration in collisionless supernovae remnant shocks: II- Cosmic-ray transport
• Cosmic-ray acceleration and escape from post-adiabatic Supernova remnants
• The nature of gamma-ray emission of Tycho's supernova remnant
• Understanding hadronic gamma-ray emission from supernova remnants
• Nonlinear shock acceleration beyond the Bohm limit
• Two-Step Acceleration Model of Cosmic Rays at Middle-Aged SNR
• Slow Diffusion of Cosmic-Rays around a Supernova Remnant
• Cosmic ray driven winds in the Galactic environment and the cosmic ray spectrum
• Diffuse γ-ray emission from self-confined cosmic rays around Galactic sources
• Dynamics of Mesoscale Magnetic Field in Diffusive Shock Acceleration
• Alfven Wave Amplification and Self-Containment of Cosmic-Rays Escaping from a Supernova Remnant
• Theory of cosmic ray and gamma-ray production in the supernova remnant RX J0852.0-4622
• Nonthermal emission of supernova remnant SN 1006 revisited: theoretical model and the H.E.S.S. results
• Gamma-ray signatures of cosmic ray acceleration, propagation, and confinement in the era of CTA
• H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloud
• Where are Milky Way's Hadronic PeVatrons?
• Reacceleration of electrons in supernova remnants
• Prospects for CTA observations of the young SNR RX J1713.7-3946
• Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble
• 3D simulations of the non-thermal broad-band emission from young supernova remnants including efficient particle acceleration
• Exploring the Gamma-Ray Emissivity of Young Supernova Remnants I: Hadronic Emission
• Expected gamma-ray emission of supernova remnant SN 1987A
• Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
• NuSTAR Detection of a Hard X-ray Source in the Supernova Remnant - Molecular Cloud Interaction Site of IC 443
• Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array
• On The Origin of Very High Energy Cosmic Rays
• Observational constraints on the maximum energies of accelerated particles in supernova remnants: low maximum energies and a large variety
• The Tunka Experiment: Towards a 1-km^2 Cherenkov EAS Array in the Tunka Valley
• Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud
• Gamma-ray emission from middle-aged supernova remnants interacting with molecular clouds: the challenge for current models
• The Contribution of Different Supernova Populations to the Galactic Gamma-Ray Background
• Localized SiO emission triggered by the passage of the W51C SNR shock
• Cosmic-ray electrons released by supernova remnants
• Fast Particle Acceleration at Perpendicular Shocks with Uniform Upstream Magnetic Field and Strong Downstream Turbulence
• Origin of Galactic Cosmic Rays from Supernova Remnants
• Study on the escape timescale of high-energy particles from supernova remnants through thermal X-ray properties
• Selected Topics in Cosmic Ray Physics
• Formation of the cosmic-ray halo: Galactic spectrum of primary cosmic rays
• Radio polarization maps of shell-type SNRs II. Sedov models with evolution of turbulent magnetic field
• Detection of gamma rays around SNR HB9 and its implication to the diffusive shock-acceleration history
• The Important Role of Cosmic-Ray Re-Acceleration
• On The {\it Fermi} -Lat Surplus of the Diffuse Galactic Gamma-Ray Emission
• Microquasar jet-cocoon systems as PeVatrons
• Multiwavelength studies of G298.6$-$0.0: An old GeV supernova remnant interacting with molecular clouds
• Gamma-ray Production in the Extended Halo of the Galaxy and Possible Implications for the Origin of Galactic Cosmic Rays
• Origin of Spectral Hardening of Secondary Cosmic-Ray Nuclei
• Probing the origin of 4FGL J0822.8-4207: cosmic ray illumination from the SNR Puppis A and the Herbig-Haro object HH219
• Modeling the multiwavelength emission from G73.9+0.9: Gamma-rays from a SNR-MC interaction
• Particle Acceleration at shocks: some modern aspects of an old problem
• Escape of cosmic rays from perpendicular shocks in the circumstellar magnetic field
• Spatially decomposed $\gamma$-ray features surrounding SNR Kes 79 & PSR J1853+0056
• The population of Galactic supernova remnants in the TeV range
• Regions of suppressed diffusion around supernova remnants?
• The Orion Region: Evidence of enhanced cosmic-ray density in a stellar wind forward shock interaction with a high density shell
• Models and phenomenology
• Reacceleration of charged dark matter
• Time-dependent escape of cosmic rays from supernova remnants potentially at the origin of the very-high-energy cosmic-ray gradient of the Galactic center
• Supernova remnants in clumpy medium: A model of hydrodynamic and radio synchrotron evolution
• PeVatron Candidate SNR G106.3+2.7 in a Low-density Cavity: a Multiwavelength Test
• The origin of ultra high energy cosmic rays
• Nonthermal processes and particle acceleration in supernova remnants
• Theoretical $\Sigma$-$D$ Relations for Shell-Type Galactic Supernova Remnants
• Morphology of supernova remnants and their halos
• Escape of cosmic rays from perpendicular shocks in the interstellar magnetic field
• Examining a hadronic $\gamma$-ray scenario for the radiative shell & molecular clouds of the old GeV supernova remnant G298.6$-$0.0
• Energy-dependent extension of the Crab Nebula as a diagnostic of ultrahigh-energy hadronic emission
• Runaway stars and the Galactic supernova remnant landscape: non-thermal emission and observational evidence