Cooling of Neutron Stars. Hadronic Model
Astrophysics
2007-05-23 v1 Nuclear Theory
Abstract
We study the cooling of isolated neutron stars. The main cooling regulators are introduced: EoS, thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. Neutrino emissivity includes main processes. A strong impact of medium effects on the cooling rates is demonstrated. With taking into account of medium effects in reaction rates and in nucleon superfluid gaps modern experimental data can be well explained.
Keywords
Cite
@article{arxiv.astro-ph/0403170,
title = {Cooling of Neutron Stars. Hadronic Model},
author = {D. Blaschke and H. Grigorian and D. N. Voskresensky},
journal= {arXiv preprint arXiv:astro-ph/0403170},
year = {2007}
}
Comments
15 pages, 23 figures, aa.cls style included