Reconciling Multi-messenger Constraints with Chiral Symmetry Restoration
Nuclear Theory
2022-08-09 v1 High Energy Astrophysical Phenomena
Abstract
We consider the parity doublet model for nucleonic and delta matter to investigate the structure of neutron stars. We show that it is possible to reconcile the multi-messenger astronomy constraints within a purely hadronic equation of state (EOS), which accounts for the self-consistent treatment of the chiral symmetry restoration in the baryonic sector. We demonstrate that the characteristics of the EOS required by the astrophysical constraints do not necessarily imply the existence of a hadron-quark phase transition in the stellar core.
Keywords
Cite
@article{arxiv.2208.03933,
title = {Reconciling Multi-messenger Constraints with Chiral Symmetry Restoration},
author = {Michał Marczenko and Krzysztof Redlich and Chihiro Sasaki},
journal= {arXiv preprint arXiv:2208.03933},
year = {2022}
}
Comments
Presented at Quark Matter 2022