From nuclear matter to Neutron Stars
Nuclear Theory
2009-02-03 v1
Abstract
Neutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.
Cite
@article{arxiv.0902.0262,
title = {From nuclear matter to Neutron Stars},
author = {T. K. Jha},
journal= {arXiv preprint arXiv:0902.0262},
year = {2009}
}
Comments
10 Figures, 1 Table