Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables
Astrophysics
2017-08-23 v2 High Energy Physics - Phenomenology
Nuclear Theory
Abstract
Depending on the density reached in the cores of neutron stars, such objects may contain stable phases of novel matter found nowhere else in the Universe. This article gives a brief overview of these phases of matter and discusses astrophysical constraints on the high-density equation of state associated with ultra-dense nuclear matter.
Keywords
Cite
@article{arxiv.0808.1279,
title = {Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables},
author = {David Blaschke and Thomas Klaehn and Fridolin Weber},
journal= {arXiv preprint arXiv:0808.1279},
year = {2017}
}
Comments
16 pages, 11 figures, Contribution to Proceedings of the 3rd International Workshop on Astronomy and Relativistic Astrophysics (IWARA), 3-6 October 2007, Joao Pessoa, Brazil