Cosmic rays & diffusive shock acceleration at highly oblique non-relativistic shocks

✍ Scribed by Athina Meli; L. Peter Biermann

Publisher: Elsevier Science
Year: 2006
Tongue: English
Weight: 167 KB
Volume: 151
Category: Article
ISSN: 0920-5632
DOI: 10.1016/j.nuclphysbps.2005.07.089

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The process of diffusive acceleration of charged particles in shocked plasmas is widely invoked in astrophysics to account for the ubiquitous presence of signatures of non-thermal relativistic electrons and ions in the universe. A key characteristic of this statistical energization mechanism is the