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Test of galactic cosmic-ray source models – Working Group Report

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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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Authors and Affiliations

  1. Dublin Institute for Advanced Studies, IRL-Dublin 2, Ireland

    L. O’C. Drury & E. Parizot

  2. Department of Physics, North Carolina State University, Raleigh, NC, 27695, U.S.A

    D.E. Ellison & S. Reynolds

  3. Max-Planck-Institut für Kernphysik, Heidelberg, Germany

    F.A. Aharonian

  4. Institute of Cosmophysical Research and Aeronomy, 677891, Yakutsk, Russia

    E. Berezhko

  5. A.F. Ioffe Institute for Physics and Technology, 194021, St. Petersburg, Russia

    A. Bykov

  6. Service d’Astrophysique, CEA Saclay, 91191, Gif-sur-Yvette, France

    A. Decourchelle

  7. Max-Planck-Institut für Extraterrestrische Physik, D-85741, Garching

    R. Diehl

  8. Geneva Observatory, 1290 Sauverny, Switzerland

    G. Meynet

  9. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA , 02138, U.S.A

    J. Raymond

  10. Dept. of Physics and Astronomy, University of Iowa, Iowa City, Iowa, 52242, U.S.A

    S. Spangler

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Drury, L.O., Ellison, D., Aharonian, F. et al. Test of galactic cosmic-ray source models – Working Group Report. Space Science Reviews 99, 329–352 (2001). https://doi.org/10.1023/A:1013825905795

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