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Combined protection from beams of high-energy μ-mesons

✍ Scribed by N. P. Kalashnikov; V. K. Lapshin; V. V. Frolov


Publisher
Springer US
Year
1974
Tongue
English
Weight
88 KB
Volume
36
Category
Article
ISSN
1573-8205

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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 Δ resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum o