Neutrinos in Neutron Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

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 γ(B)
integrated by Tsuruta and Cameron (1966b) 1%. As a result a neutrino sea
is formed and some radioactive isotopes may become stable.

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