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Non-thermal acceleration mechanisms in supernova remnant shells
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Mem. S.A.It. Vol. 75, 282
c? SAIt 2004 Memorie della
Non-thermal a
eleration me
hanisms insupernova remnant shells
A. Decourchelle
1
Laboratoire AIM, CEA/DSM - CNRS - Universite? Paris Diderot, DAPNIA/Service
d’Astrophysique, Ba?t. 709, CEA-Saclay, F-91191 Gif-sur- Yvette Ce?dex, France e-mail:
anne.decourchelle@cea.fr
Abstract. A 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 observa-
tions of supernova remnants in hard X-rays and in gamma rays. Open issues are discussed
in this framework.
Key words. ISM: supernova remnants – X-rays: ISM – Gamma rays: observations –
Acceleration of particles – Radiation mechanisms: non-thermal – Shock waves –
1. Introduction
Supernova remnants (SNRs) are expected to
be the main source of cosmic rays with ener-
gies up to the knee at ? 3 1015 eV (see for
a discussion Drury et al. 2001). The ejection
of high velocity material during the explosion
gives rise to a shock that both heats the ambi-
ent medium to millions degrees and accelerates
particles.
While the millions degrees gas emits ther-
mal X-rays below 10 keV, the accelerated
charged particles produce non-thermal emis-
sion over the entire electromagnetic spectrum
through four main emission mechanisms. First,
the accelerated electrons produce synchrotron
emission when spiraling in a magnetic field.
This emission, extending from the radio to X-
ray domains, corresponds to a population of
GeV and TeV accelerated electrons, respec-
tively. The population of TeV electrons, ob-
Send offprint requests to: A. Decourchelle
served in X-ray synchrotron, gives also rise to
Inverse Compton emission: they communicate
a large part of their energy to low energy pho-
tons (from the Cosmic Microwave Background
or from the l
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