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Test of Galactic Cosmic-Ray source models - Working group report

Abstract : The main features of cosmic-ray source models and acceleration processes are reviewed, with special emphasis on the possible observational tests, through both composition analysis and multi-wavelength studies of supernova remnants. Non-linear effects in the context of supernova-induced diffusive shock acceleration are discussed, as well as collective acceleration effects induced by multiple supernova explosions inside superbubbles.
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Contributor : Suzanne Robert <>
Submitted on : Monday, March 11, 2002 - 3:19:42 PM
Last modification on : Wednesday, September 16, 2020 - 4:01:53 PM

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Lo. Drury, De. Ellison, Fa. Aharonian, E. Berezhko, A. Bykov, et al.. Test of Galactic Cosmic-Ray source models - Working group report. ISSI Workshops The Astrophysics of Galactic Cosmic Rays, May 2000, Berne, Switzerland. pp.329-352. ⟨in2p3-00011710⟩



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