中子星冷却理论与观测的对比
天体物理学
2008-11-26 v2
摘要
我们回顾了中子星冷却理论的现状，并讨论了通过将冷却理论与孤立中子星热辐射观测进行对比，从而限制中子星核心的物态方程、中微子发射和超流性质的前景。
引用
@article{arxiv.0710.2047,
title = {Theory of cooling neutron stars versus observations},
author = {D. G. Yakovlev and O. Y. Gnedin and A. D. Kaminker and A. Y. Potekhin},
journal= {arXiv preprint arXiv:0710.2047},
year = {2008}
}
备注
9 pages, 4 figures, 3 tables, to appear in the proceedings of "40 Years of Pulsars" held in Montreal, Canada, August 12-17, 2007, eds. C. Bassa, Z. Wang, A. Cumming, V. Kaspi, AIP, in press (v.2 - minor bibliography corrections)