High energy neutrinos from the tidal disruption of stars
نویسندگان
چکیده
منابع مشابه
Production of high-energy μ neutrinos from young neutron stars
Young, rapidly rotating neutron stars could accelerate protons to energies of ∼ 1 PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the ∆ resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum of muon neutrinos consists of a sharp rise at ∼ 50 TeV, corresponding to the onset of the resonanc...
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ژورنال
عنوان ژورنال: Physical Review D
سال: 2017
ISSN: 2470-0010,2470-0029
DOI: 10.1103/physrevd.95.123001