中子星退禁闭相变加热与热演化
天体物理学
2008-11-26 v2
摘要
若退禁闭相变为一阶相变，则在中子星自转减慢过程中，该相变将导致潜热的释放。我们研究了经历此类退禁闭相变的中子星的热演化。结果表明，中子星可能被加热至更高的温度。这一特征对于晚期低磁场毫秒脉冲星的高温现象尤为有趣。
引用
@article{arxiv.0711.0443,
title = {Deconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars},
author = {Miao Kang and Nana Pan and Xiaodong Wang},
journal= {arXiv preprint arXiv:0711.0443},
year = {2008}
}
备注
4 pages, to be published by American Institute of Physics, ed. D.Lai, X.D.Li and Y.F.Yuan, as the Proceedings of the conference Astrophysics of Compact Objects