Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications
Nuclear Theory
2021-01-26 v2 High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
Abstract
In the current work an equation of state model with a first-order phase transition for astrophysical applications is presented. The model is based on a two-phase approach for quark-hadron phase transitions, which leads by construction to a first-order phase transition. The resulting model has already been successfully used in several astrophysical applications, such as cold neutron stars, core-collapse supernova explosions and binary neutron star mergers. Main goal of this work is to present the details of the model, discuss certain features and eventually publish it in a tabulated form for further use.
Keywords
Cite
@article{arxiv.2009.10846,
title = {Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications},
author = {Niels-Uwe F. Bastian},
journal= {arXiv preprint arXiv:2009.10846},
year = {2021}
}