Detection of neutrinos from microquasares.II

M.MOSQUERA; O. CIVITARESE

INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS

WORLD SCIENTIFIC PUBL CO PTE LTD

Lugar: London, UK; Año: 2012 vol. 21 p. 1250086 - 1250096

0218-3013

Considering a system composed of a compact object and a star subrounded by wind,and using models for high-energy proton emission from micro-quasars, we calculate theneutrino flux resulting from proton–proton collisions, with and without including neu-trino oscillations. It is found that the flux of neutrinos from a windy micro-quasar isaffected by neutrino oscillations, and that it reflects upon the increase in the time ofobservation, by a factor of the order 2–3.