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Cited by 1,967

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Particle acceleration by astrophysical shocks

Blandford, R. D., Ostriker, J. P.·1978·The Astrophysical Journal

Abstract

A new mechanism is proposed for acceleration of a power-law distribution of cosmic rays with approximately the observed slope. High-energy particles in the vicinity of a shock are scattered by Alfven waves carried by the converging fluid flow leading to a first-order acceleration process in which the escape time is automatically comparable to the acceleration time. Shocks from supernova explosions propagating through the interstellar medium can account for the acceleration of galactic cosmic rays. Similar processes occurring in extragalactic radio sources can lead to efficient in situ acceleration of relativistic electrons.

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Metadata

Authors
Blandford, R. D., & Ostriker, J. P.
Venue
The Astrophysical Journal
Published
1978-04
Volume
221
Pages
L29
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2069414247
Cited by
1,967
References
0
FWCI
9.39
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Particle acceleration by astrophysical shocks. https://app.cochat.ai/papers/10.1086/182658
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Blandford, R. D., & Ostriker, J. P. (1978). Particle acceleration by astrophysical shocks. The Astrophysical Journal. https://doi.org/10.1086/182658

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.