Neutrino Mean Free Path in Neutron Stars
Nuclear Theory
2009-11-07 v3
Abstract
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.
Keywords
Cite
@article{arxiv.nucl-th/0212037,
title = {Neutrino Mean Free Path in Neutron Stars},
author = {U. Lombardo and Caiwan Shen and N. Van Giai and W. Zuo},
journal= {arXiv preprint arXiv:nucl-th/0212037},
year = {2009}
}
Comments
6 pages, 8 figures, for proceeding of International Symposium on Physics of Unstable Nuclei, Halong Bay(Vietnam) Nov. 2002. Espcrc1.sty is given