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Neutrinos in neutron stars
Authors:Osmi Vilhu
Institution:(1) Astrophysics Laboratory, University of Helsinki, Finland
Abstract:It is shown that in neutron stars some of the neutrinos cannot escape from the star. For incompressible fluid sphere models, this part, in the optimum case, is 25%, and for the modelV gamma(B) integrated byTsuruta andCameron (1966b) 1%. As a result a neutrino sea is formed and some radioactive isotopes may become stable.
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