Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1968
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968ap%26ss...1..301v&link_type=abstract
Astrophysics and Space Science, Volume 1, Issue 3, pp.301-308
Astronomy and Astrophysics
Astrophysics
3
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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