Effects of rotochemical heating on the thermal evolution of superfluid neutron stars
High Energy Astrophysical Phenomena
2010-05-26 v1
Abstract
The authors take the rotochemical heating effect into account, which may make the cooling scenario different. Their model is consistent with the observation data.
Cite
@article{arxiv.1005.4473,
title = {Effects of rotochemical heating on the thermal evolution of superfluid neutron stars},
author = {Chun-Mei Pi},
journal= {arXiv preprint arXiv:1005.4473},
year = {2010}
}
Comments
7 pages, 2 figures. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at Peking University, Beijing - P. R. China [http://vega.bac.pku.edu.cn/rxxu/csqcd.htm]