从中子星到奇异星
天体物理学
2007-05-23 v1
摘要
本文讨论了 strange quark matter 可能的绝对稳定性所引发的若干最有趣的天体物理意义。随后讨论了两种天体信号，这两种信号可能指向 strange quark matter 存在于孤立中子星以及低质量 X 射线二氧化碳星 (LMXB) 中的中子星。
引用
@article{arxiv.astro-ph/0112058,
title = {From Neutron Stars to Strange Stars},
author = {Fridolin Weber},
journal= {arXiv preprint arXiv:astro-ph/0112058},
year = {2007}
}
备注
Paper presented at the int. conference "Compact Stars in the QCD Phase Diagram", held in Copenhagen (NORDITA - Niels Bohr Institute), August 15-18, 2001; organized by Rachid Ouyed and Francesco Sannino; (12 pages, 6 figures)