High Energy CRs from Young Neutron Star and Their Interactions with the Ambient Matter

Details High Energy CRs from Young Neutron Star and Their Interactions with the Ambient Matter High Energy CRs from Young Neutron Star and Their Interactions with the Ambient Matter

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2..703n&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

We have estimated the flux of gamma-rays and neutrinos that are produced from the decays of neutral and charged pions in the pulsar winds. The number density and energy spectrum of pions have been calculated assuming that the distribution of the protons in the downstream of the standing shock wave is a Maxwellian with very high temperature and high energy protons interact with each other. We compared the estimated flux of gamma-rays with the observed one for the Crab Nebula and discussed the possibility to detect the signals of high energy neutrino at km3 detector such as IceCub e.

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