Cooling of hybrid neutron stars with microscopic equations of state
Nuclear Theory
2020-10-12 v1 High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
Abstract
We model the cooling of hybrid neutron stars combining a microscopic nuclear equation of state in the Brueckner-Hartree-Fock approach with different quark models. We then analyze the neutron star cooling curves predicted by the different models and single out the preferred ones. We find that the possibility of neutron p-wave pairing can be excluded in our scenario.
Keywords
Cite
@article{arxiv.2003.08079,
title = {Cooling of hybrid neutron stars with microscopic equations of state},
author = {J. -B. Wei and G. F. Burgio and H. -J. Schulze and and D. Zappalà},
journal= {arXiv preprint arXiv:2003.08079},
year = {2020}
}
Comments
10 pages, 6 figures