Neutrino Mean Free Path in Neutron Stars
arXiv:nucl-th/0212037 · doi:10.1016/S0375-9474(03)01422-2
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.
arXiv comment6 pages, 8 figures, for proceeding of International Symposium on Physics of Unstable Nuclei, Halong Bay(Vietnam) Nov. 2002. Espcrc1.sty is given
References in corpus (2)
Cited by in corpus (5)
- Isospin splitting of the nucleon mean field
- 1S0 Proton and Neutron Superfluidity in beta-stable Neutron Star Matter
- Neutrino mean free path in neutron stars
- Microscopic calculation of neutrino mean free path inside hot neutron matter
- Three-body force effect on neutrino emissivities of neutron stars within the framework of the Brueckner-Hartree-Fock approach