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On the Shape of the Spectrum of Cosmic-rays Accelerated inside Superbubbles
Ferrand G., Marcowith A.
Astronomy & Astrophysics 510, A101 (2010) pp - http://hal.archives-ouvertes.fr/hal-00435196
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Physique/Astrophysique/Phénomènes cosmiques de haute energie
Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
On the Shape of the Spectrum of Cosmic-rays Accelerated inside Superbubbles
Gilles Ferrand ()1, Alexandre Marcowith ()2
1 :  SAp - Service d'Astrophysique
http://www-dapniai2.cea.fr/Dapnia/Sap/Fr/homepage.php
CEA : DSM/IRFU
Service d'Astrophysique, CEA-Saclay, DSM/DAPNIA/SAp, Bât. 709, L'Orme des Merisiers, F-91 191 Gif-sur-Yvette Cedex, France
France
2 :  LPTA - Laboratoire de Physique Théorique et Astroparticules
http://www.lpta.in2p3.fr/
CNRS : UMR5207 – IN2P3 – Université Montpellier II - Sciences et techniques
Bât 13- 1er Et. - CC 070 Place Eugène Bataillon 34095 MONTPELLIER CEDEX 5
France
Supernova remnants are believed to be a major source of cosmic-rays in the Galaxy. As their progenitors are commonly found clustered in OB associations, one has to consider the possibility of collective effects in the acceleration process. In this work we investigate the shape of the spectrum of protons accelerated inside the superbubbles blown around clusters of massive stars. To do so we embed semi-analytical models of particle acceleration and transport inside Monte-Carlo simulations of OB associations timelines. We consider regular acceleration at the shock front of supernova remnants, as well as stochastic re-acceleration and escape occurring between the shocks. We observe that particle spectra, although strongly intermittent, get a distinctive shape resulting from a competition between acceleration and escape: they are harder at the lowest energies and softer at the highest energies. The momentum at which this spectral break occurs depends on a single dimensionless parameter, which we evaluate for a selection of objects. The behaviour of a superbubble regarding acceleration depends on the magnetic turbulence: if B is low the superbubble is simply the host of a collection of individual supernovae shocks, but if B is high enough it acts as a global accelerator, producing distinctive spectra – which has important implications on the high-energy emission from these objects.
Anglais
21/10/2009

Astronomy & Astrophysics
internationale
Articles dans des revues avec comité de lecture
26/02/2010
510
A101
pp

acceleration of particles – shock waves – turbulence – cosmic rays – supernova remnants
11 p.
09-088

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/0911.4457
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