Non-thermal acceleration mechanisms in supernova remnant shells

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dc.creatorDecourchelle, Anne
dc.date2008-02-04
dc.date.accessioned2026-07-07T09:18:33Z
dc.date.available2026-07-07T09:18:33Z
dc.descriptionA review of the main issues in the field of particle acceleration in Supernova Remnants is provided in the context of future X-ray observations with Simbol-X. After a summary of the nonthermal acceleration mechanisms at work, I briefly review the observations of supernova remnants in hard X-rays and in gamma rays. Open issues are discussed in this framework.
dc.description6 pages, 3 figures, invited talk at 'Simbol-X: the hard X-ray universe in focus', Bologna (Italy), 14-16 May, 2007. To appear in Memorie della SAIt
dc.identifierhttps://arxiv.org/abs/0802.0372
dc.identifierhttp://arxiv.org/abs/0802.0372
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/154064
dc.subjectAstrophysics
dc.titleNon-thermal acceleration mechanisms in supernova remnant shells
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