Physics
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..713b&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Aug. 1988, p. 713-724. In Russian. In Russian.
Physics
1
Gamma Rays, Neutrinos, Shock Waves, Supernovae, X Rays, Acceleration (Physics), Cosmic Rays, Relativistic Particles, Shock Fronts, Stellar Envelopes, Stellar Winds
Scientific paper
Gamma, neutrino and X-ray radiation produced by relativistic protons are considered. Proton acceleration occurs at the fronts of two strong shocks that limit the transition region between the flying away envelope of young SN II and the presupernova wind material. The protons are effectively confined in this transition region and give radiation via pion decays due to interaction with the gas. X-ray radiation is given as lower limit provided by secondary electrons. The fluxes of gamma, neutrino and X-ray radiation expected from SN II in our Galaxy are shown to be detectable. The signature of the considered mechanisms is early production of the signal at 10 - 100 days after the SN explosion.
Berezinsky Veniamin S.
Ptuskin Vladimir S.
No associations
LandOfFree
Radiation from the young envelopes of type II supernovae, generated by shock-accelerated cosmic rays does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radiation from the young envelopes of type II supernovae, generated by shock-accelerated cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation from the young envelopes of type II supernovae, generated by shock-accelerated cosmic rays will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1695534