中子星磁场：理论视角
天体物理学
2009-11-10 v1
摘要
我们提出了关于决定中子星磁场演化的主要物理要素的观点。这包括中子星物质的基本性质、磁场起源的可能情景、其演化的约束与机制，以及对我们近期关于霍尔漂移工作的讨论。
引用
@article{arxiv.astro-ph/0503047,
title = {Magnetic fields in neutron stars: A theoretical perspective},
author = {Andreas Reisenegger and Joaquin Prieto and Rafael Benguria and Dong Lai and Pablo Araya},
journal= {arXiv preprint arXiv:astro-ph/0503047},
year = {2009}
}
备注
Invited review, conference "Magnetic Fields in the Universe: from Laboratory and Stars to Primordial Structures", Angra dos Reis, Brazil, Nov 28 - Dec 3, 2004, eds. E. M. de Gouveia dal Pino, A. Lazarian, & G. Lugones, to be published in the AIP COnference Proceedings. 11 pages, no figures