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High-energy emission from presupernovae

✍ Scribed by Volodymyr Kryvdyk

Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
162 KB
Volume
33
Category
Article
ISSN
0273-1177

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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