Gamma-Rays and Neutrinos from the Pulsar Wind Nebulae

Details Gamma-Rays and Neutrinos from the Pulsar Wind Nebulae Gamma-Rays and Neutrinos from the Pulsar Wind Nebulae

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2481b&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 construct the time dependent radiation model for the pulsar wind nebulae (PWNe), assuming that leptons are accelerated in resonant scattering with heavy nuclei, which are injected into the nebula by the pulsar. We calculate the equilibrium spectra of these particles inside the nebula taking into account their radiation and adiabatic energy losses. The spectra of γ -rays are compared with the observations of the PWNe emitting TeV γ -rays and predictions are made for the expected γ -ray fluxes from other PWNe. expected neutrino fluxes and neutrino event rates in a 1 km2 neutrino detector from these nebulae are also calculated. It is found that only the Crab Nebula, and possibly the Vela nebula and MSH15-52, can produce detectable neutrino event rates.

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