Neutrino Mean Free Path in Neutron Stars

Details Neutrino Mean Free Path in Neutron Stars Neutrino Mean Free Path in Neutron Stars

2002-12-06

arxiv.org/abs/nucl-th/0212037v3

Nucl.Phys. A722 (2003) 532-537

Physics

Nuclear Physics

Nuclear Theory

6 pages, 8 figures, for proceeding of International Symposium on Physics of Unstable Nuclei, Halong Bay(Vietnam) Nov. 2002. Es

Scientific paper

10.1016/S0375-9474(03)01422-2

The Landau parameters of nuclear matter and neutron matter are extracted from
the Brueckner theory including three-body forces. The dynamical response
function to weak neutrino current is calculated in terms of the Landau
Parameters in the RPA limit. Then, the neutrino mean free path in neutron stars
is calculated for different conditions of density and temperature.

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