Comparing neutron star predictions by various microscopic models
Nuclear Theory
2009-06-02 v1
Abstract
We calculate several neutron star properties, for static and/or rotating stars, using equations of state based on different microscopic models. These include our Dirac-Brueckner-Hartree-Fock model and others derived from the non-relativistic Brueckner-Hartree-Fock approach implemented with microscopic three-body forces. The model dependence is discussed.
Cite
@article{arxiv.0906.0320,
title = {Comparing neutron star predictions by various microscopic models},
author = {F. Sammarruca and Pei Liu},
journal= {arXiv preprint arXiv:0906.0320},
year = {2009}
}
Comments
8 pages, 8 figures, revtex4