旋转化学加热对超流中子星热演化的影响
高能天体物理现象
2010-05-26 v1
摘要
作者考虑了旋转化学加热效应，该效应可能使冷却情景有所不同。他们的模型与观测数据一致。
引用
@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}
}
备注
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]