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

Drury, L. O.; Ellison, D. E.; Aharonian, F. A.; Berezhko, E.; Bykov, A.; Decourchelle, A.; Diehl, R.; Meynet, G.; Parizot, E.; Raymond, J.; Reynolds, S.; Spangler, S.

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

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Aharonian, F. A.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Drury, L. O., Ellison, D. E., Aharonian, F. A., Berezhko, E., Bykov, A., Decourchelle, A., et al. (2001). Test of Galactic Cosmic-Ray source models - Working group report. Space Science Reviews, 99(1-4), 329-352.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-856B-8

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.