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The acceleration of cosmic rays in shock fronts – I

A. R. Bell
- 01 Feb 1978 - 
- Vol. 182, Iss: 2, pp 147-156
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1978-02-01 and is currently open access. It has received 2613 citations till now. The article focuses on the topics: Shock waves in astrophysics & Fermi acceleration.

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Journal ArticleDOI

Radio signature of cosmological structure formation shocks

TL;DR: In this paper, the authors derived an analytic expression for the total radio power in the downstream region of a cosmological shock wave, and the width of the radio-emitting region.
Journal ArticleDOI

The Origin of Galactic Cosmic Rays

TL;DR: In this article, the authors present a review of the theory of diffusive particle acceleration at supernova remnant shocks, with special attention for the dynamical reaction of accelerated particles on the shock and the phenomenon of magnetic field amplification at the shock.
Journal ArticleDOI

Filamentation Instability of Counterstreaming Laser-Driven Plasmas

TL;DR: Filamentation due to the growth of a Weibel-type instability was observed in the interaction of a pair of counterstreaming, ablatively driven plasma flows, in a supersonic, collisionless regime relevant to astrophysical collisionless shocks.
Journal ArticleDOI

Neutrino Afterglow from Gamma-Ray Bursts: ~1018 eV

TL;DR: In this article, it was shown that a significant fraction of the energy of a γ-ray burst (GRB) is probably converted to a burst of 1017-1019 eV neutrinos and multiple GeV γ rays that follow the main GRB by ~10 s.
Journal ArticleDOI

Ultra-high-energy cosmic ray acceleration by relativistic blast waves

TL;DR: In this article, the acceleration of charged particles at the ultrarelativistic shocks, with Lorentz factors Γs≫1 relative to the upstream medium, arising in relativistic fireball models of gamma-ray bursts (GRBs), was considered.
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