Equation of State at High-Baryon Density and Compact Stellar Objects
Nuclear Theory
2022-07-01 v1 High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
Abstract
In this contribution I review the connection between compact stars and high-baryon density matter, focusing on astrophysical observables for deconfinement to quark matter. I discuss modern ingredients, repositories, and constraints for the neutron-star equations of state. Finally, I draw comparisons between dense and hot matter created in neutron-star mergers and heavy-ion collisions, and the possibility of quantitatively establishing a link between them.
Cite
@article{arxiv.2206.14963,
title = {Equation of State at High-Baryon Density and Compact Stellar Objects},
author = {Veronica Dexheimer},
journal= {arXiv preprint arXiv:2206.14963},
year = {2022}
}
Comments
Presented at Quark Matter 2022