GLAST simulation study of an extended TeV-emitting supernova remnant for the origin of cosmic-ray nuclei

Details GLAST simulation study of an extended TeV-emitting supernova remnant for the origin of cosmic-ray nuclei GLAST simulation study of an extended TeV-emitting supernova remnant for the origin of cosmic-ray nuclei

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..921..397k&link_type=abstract

THE FIRST GLAST SYMPOSIUM. AIP Conference Proceedings, Volume 921, pp. 397-398 (2007).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Supernova Remnants, Cosmic Rays

Scientific paper

We extracted the gamma-ray emission of the π0-decay, which will be a
decisive evidence of cosmic-ray proton acceleration, from the one-year
data of an extended TeV-emitting supernova remnant, generated by the
GLAST full detector simulation, although many assumptions were
oversimplified.

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