Effects of rotochemical heating on the thermal evolution of superfluid neutron stars
arXiv:1005.4473
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.
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]