Cosmic ray acceleration and escape from supernova remnants

Abstract

Galactic cosmic ray (CR) acceleration to the knee in the spectrum at a few PeV is only possible if the magnetic field ahead of a supernova remnant (SNR) shock is strongly amplified by CR escaping the SNR. A model formulated in terms of the electric charge carried by escaping CR predicts the maximum CR energy and the energy spectrum of CR released into the surrounding medium. We find that historical SNR such as Cas A, Tycho and Kepler may be expanding too slowly to accelerate CR to the knee at the present time.

17 pages, 5 figures, accepted for publication in the Monthly Notices of the Royal Astronomical Society

References in corpus (9)

• Circumstellar Emission from Type Ib and Ic Supernovae
• Diffusive Shock Acceleration with Magnetic Amplification by Non-resonant Streaming Instability in SNRs
• Confirmation of strong magnetic field amplification and nuclear cosmic ray acceleration in SN 1006
• Nonlinear Diffusive Shock Acceleration with Magnetic Field Amplification
• Dynamical Feedback of Self-generated Magnetic Fields in Cosmic Ray Modified Shocks
• Modeling Bell's Non-resonant Cosmic Ray Instability
• Universal behaviour of shock precursors in the presence of efficient cosmic-ray acceleration
• Cosmic ray diffusion near the Bohm limit in the Cassiopeia A supernova remnant
• Cosmic ray current-driven turbulence and mean-field dynamo effect

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