Pulsars Covered by the Dense Envelopes as High-Energy Neutrino Sources

Details Pulsars Covered by the Dense Envelopes as High-Energy Neutrino Sources Pulsars Covered by the Dense Envelopes as High-Energy Neutrino Sources

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pthph..58..549s&link_type=abstract

Progress of Theoretical Physics, Vol. 58, No. 2, pp. 549-559

Physics

32

Scientific paper

A newly-born pulsar is covered by the expanding dense envelope, and high-energy charged particles accelerated near the pulsar are effectively converted into high-energy neutrinos with energies of 1013 ˜ 1014 eV through meson production and its decay. Such a opaque phase continues for a couple of months. This model was first proposed by Berezinsky, but we will show that his flux estimation is too high by a factor of ˜ 105. This reduction is needed because the particle flux is limited by the accompanying phenomena such as the source power of high-energy cosmic rays and the light element production rate by spallation nuclear reaction.

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