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High-energy emission from millisecond pulsars: polar cap models

โœ Scribed by Qinghuan Luo; Shinpei Shibata; Donald B. Melrose


Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
218 KB
Volume
318
Category
Article
ISSN
0035-8711

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High energy neutrino emission from young
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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