Inner crust equations of state for CompOSE
Nuclear Theory
2022-09-07 v1 High Energy Astrophysical Phenomena
Abstract
In this paper, we present some relativistic mean-field inner crust equations of state that have recently been uploaded in the CompOSE online repository. These equations of state fulfill experimental and microscopic constraints, and are also able to reproduce two solar-mass stars. We integrate the TOV equations to obtain the mass-radius relation, and we also calculate the tidal deformability, compactness, and effective tidal deformability to compare with the latest astrophysical data from NICER and LIGO and Virgo.
Cite
@article{arxiv.2207.14153,
title = {Inner crust equations of state for CompOSE},
author = {Tuhin Malik and Helena Pais},
journal= {arXiv preprint arXiv:2207.14153},
year = {2022}
}
Comments
13 pages, 5 figures, 3 tables, accepted for publication in the EPJA's Topical Issue "CompOSE: a repository for Neutron Star Equations of State and Transport Properties"