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Neutrinos from binary pulsars

โœ Scribed by EICHLER, DAVID

Book ID
109711055
Publisher
Nature Publishing Group
Year
1978
Tongue
English
Weight
261 KB
Volume
275
Category
Article
ISSN
0028-0836

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We propose that young (t age t10 5 yr), rapidly rotating pulsars can accelerate ions to energies of $1 PeV near the surface of a neutron star. Protons undergo resonant excitation with surface X-rays and produce a beam of m neutrinos with energies of several tens of TeV which could be detectable by c