中子星——冷却与输运
高能天体物理现象
2017-10-19 v3 太阳与恒星天体物理
摘要
借助中子星热演化理论，对中子星热辐射的观测有可能提供关于这些星体内部超核密度物质状态的信息。我们综述了具有强磁场的孤立中子星这一理论的基础，包括星核、地壳和覆盖包层中最相关的热力学与动力学性质。
引用
@article{arxiv.1507.06186,
title = {Neutron stars - cooling and transport},
author = {A. Y. Potekhin and J. A. Pons and Dany Page},
journal= {arXiv preprint arXiv:1507.06186},
year = {2017}
}
备注
57 pages, 3 tables, 12 figures, invited topical review in The Strongest Magnetic Fields in the Universe, eds. V. S. Beskin, A. Balogh, M. Falanga, M. Lyutikov, S. Mereghetti, T. Piran, R. A. Treumann (Space Sciences Series of ISSI, Springer). In v.2, a typo in Eq.(3) is fixed. In v.3, Eqs.(32)-(33) are corrected, and references updated