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A&A Supplement series, Vol. 129, April II 1998, 343-351
Received March 26; accepted October 2, 1997
J.A. Pons
- J.A. Miralles
-
J.M
Ibáñez![]()
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Departament d'Astronomia i Astrofısica, Universitat de Valencia
46100 Burjassot (Valencia), Spain
Astronomy program, Department of Physics and Astronomy, SUNY at
Stony Brook, Stony Brook, New York 11794, U.S.A.
We calculate the Legendre expansion of the rate of the
process
up to
order
extending previous
results of other authors which only consider the
and
order terms.
Using different closure relations for the moment equations of
the radiative transfer equation we
discuss the physical implications
of taking into account quadratic and cubic terms
on the energy deposition outside the neutrinosphere in a simplified
model. The main conclusion is that
order is necessary
in the semi-transparent region and gives good results if an appropriate
closure relation is used.
keywords: radiation mechanisms: thermal -- radiative transfer -- stars: neutron -- supernovae: general -- nuclear reactions