Neutron star properties from modern meson-exchange potential models
Nuclear Theory
2009-10-22 v1
Abstract
We calculate the total mass, radius, moment of inertia and surface gravitational redshift for neutron stars using various equations of state. The latter are derived from recent meson-exchange potential models, employing both a relativistic and a non-relativistic Brueckner-Hartree-Fock approach.
Cite
@article{arxiv.nucl-th/9309021,
title = {Neutron star properties from modern meson-exchange potential models},
author = {Bao and Engvik and Hjorth-Jensen and Osnes and Oestgaard},
journal= {arXiv preprint arXiv:nucl-th/9309021},
year = {2009}
}
Comments
28 pages, elsevier latex style, report UIO-Phys-93-46