科研之友
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摘要
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 the neutrino flux resulting from proton-proton collisions, with and without including neutrino oscillations. It is found that the flux of neutrinos from a windy micro-quasar is affected by neutrino oscillations, and that it reflects upon the increase in the time of observation, by a factor of the order 2-3.
- 出版日期2012-10
