Neutrinos produced by nuclei injected by young pulsars inside compact massive binaries

Details Neutrinos produced by nuclei injected by young pulsars inside compact massive binaries Neutrinos produced by nuclei injected by young pulsars inside compact massive binaries

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nuphs.143..531b&link_type=abstract

Nuclear Physics B Supplement, Volume 143, p. 531-531.

Physics

Nuclear Physics

Scientific paper

We consider propagation of relativistic heavy nuclei injected by a young pulsar into the radiation field of a massive companion. If the binary system (BS) is compact enough, then the nuclei suffer multiple photodisintegrations in collisions with thermal photons coming from the massive star (MS). Due to the propagation effects of charged particles in the magnetic field of the MS some hadrons can impinge onto the MS surface at large angles. We calculate the fluxes of produced neutrinos as a function of the viewing angle measured from the plane of the BS. It is found that significant fluxes of neutrinos should be also expected in the case of non-eclipsing BSs.

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