Computer Science
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ssrv...99..329d&link_type=abstract
Space Science Reviews, v. 99, Issue 1/4, p. 329-352 (2001).
Computer Science
44
Scientific paper
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.
Aharonian Felix A.
Berezhko Evgeny
Bykov Andrei
Decourchelle Anne
Diehl Roland
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