Structure of the hadron-quark mixed phase in protoneutron stars
Solar and Stellar Astrophysics
2015-06-15 v1 Nuclear Theory
Abstract
We study the hadron-quark phase transition in the interior of hot protoneutron stars, combining the Brueckner-Hartree-Fock approach for hadronic matter with the MIT bag model or the Dyson-Schwinger model for quark matter. We examine the structure of the mixed phase constructed according to different prescriptions for the phase transition, and the resulting consequences for stellar properties. We find important effects for the internal composition, but only very small influence on the global stellar properties.
Keywords
Cite
@article{arxiv.1302.6074,
title = {Structure of the hadron-quark mixed phase in protoneutron stars},
author = {H. Chen and G. F. Burgio and H. -J. Schulze and N. Yasutake},
journal= {arXiv preprint arXiv:1302.6074},
year = {2015}
}
Comments
6 pages, 4 figures