Energy Spectra of High Energy Neutrinos and Cosmic Rays from Pulsars | Zendy

T. Hara | Zendy; H. Sato | Zendy

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Energy Spectra of High Energy Neutrinos and Cosmic Rays from Pulsars

Author(s) -

T. Hara,

H. Sato

Publication year - 1979

Publication title -

progress of theoretical physics

Language(s) - English

Resource type - Journals

eISSN - 1347-4081

pISSN - 0033-068X

DOI - 10.1143/ptp.62.969

Subject(s) - physics , pulsar , neutrino , cosmic ray , astrophysics , flux (metallurgy) , astronomy , spectral line , ultra high energy cosmic ray , cosmic neutrino background , energy flux , nuclear physics , neutrino detector , neutrino oscillation , materials science , metallurgy

~ 1016 e V may be generated during a few months after the birth of a pulsar, through the nuclear collisions of high energy particles generated at the pulsar with dense envelope matter. The permissible maximum flux of such neutrinos is estimated phenomenologically under a constraint that the flux of the particles ejected into the Galactic pool does not exceed the observed flux of the Galactic cosmic rays. For reason able choices of the parameters, the neutrino flux is too small to be detectable by the DUMAND project.

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