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Particle acceleration in relativistic outflows

  • In this review we confront the current theoretical understanding of particle acceleration at relativistic outflows with recent observational results on various source classes thought to involve such outflows, e.g. gamma-ray bursts, active galactic nuclei, and pulsar wind nebulae. We highlight the possible contributions of these sources to ultra-high-energy cosmic rays.

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Metadaten
Author:Andrei Bykov, Neil Gehrels, Henric Krawczynski, Martin Lemoine, Guy Pelletier, Martin PohlORCiDGND
DOI:https://doi.org/10.1007/s11214-012-9896-y
ISSN:0038-6308 (print)
Parent Title (English):Space science reviews
Publisher:Springer
Place of publication:Dordrecht
Document Type:Review
Language:English
Year of first Publication:2012
Year of Completion:2012
Release Date:2017/03/26
Tag:Cosmic rays; Particle acceleration; Shocks
Volume:173
Issue:1-4
Pagenumber:31
First Page:309
Last Page:339
Funder:Russian government [11.G34.31.0001]; RAS; RAS Presidium; RFBR [11-02-12082]; Helmholtz Alliance for Astroparticle Phyics HAP; Initiative and Networking Fund of Helmholtz Association; PEPS/PTI program of CNRS-INP
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
Peer Review:Referiert