Gamma-ray emission from SN 1006 due to accelerated cosmic rays

Details Gamma-ray emission from SN 1006 due to accelerated cosmic rays Gamma-ray emission from SN 1006 due to accelerated cosmic rays

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2489b&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to describe the properties of the remnant of SN 1006. The calculated expansion law and the radio-, X-ray and γ-ray emission produced in SN 1006 by accelerated CRs agree quite well with the observations. The π0 -decay γ-rays, generated by the nuclear CR component, dominate over the IC γ-ray component, generated by CR electrons in the inverse Compton (IC) process on the cosmic microwave background, in the observed TeV γ-ray flux from SN 1006. The predicted integral γ-ray flux Fγ ∝ -1 γ extends up to energies ˜ 100 TeV if CR diffusion is as strong as the Bohm limit.

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