Superfluidity in beta-stable neutron star matter
Nuclear Theory
2009-01-23 v1
Abstract
In this work we present results for pairing gaps in --stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results are given for superconducting protons and and neutron superfluids. A comparison is made with recent non--relativistic calculations and the implications for neutron star cooling are discussed.
Cite
@article{arxiv.nucl-th/9604041,
title = {Superfluidity in beta-stable neutron star matter},
author = {Oe. Elgaroey and L. Engvik and M. Hjorth-Jensen and E. Osnes},
journal= {arXiv preprint arXiv:nucl-th/9604041},
year = {2009}
}
Comments
7 pages, RevTex latex style, 3 figs included