夸克-介子耦合模型中的K介子凝聚与致密星
天体物理学
2009-11-11 v1
摘要
在夸克-介子耦合模型中，计算了由强子壳层和内部强子与K介子凝聚组成的中子星的性质。我们考虑了仅含核子的强子相恒星，也考虑了含超子的恒星。结果与强子相的非线性Walecka模型得到的结果进行了比较。
引用
@article{arxiv.astro-ph/0506195,
title = {Probing 3-D matter distribution at z~2 with QSO multiple lines of sight},
author = {S. Cristiani and V. D'Odorico and F. Saitta and M. Viel and S. Bianchi and B. Boyle and S. Lopez and J. Maza and P. Outram},
journal= {arXiv preprint arXiv:astro-ph/0506195},
year = {2009}
}
备注
Poster paper presented at the IAU Colloquium #199 on "Probing Galaxies through Quasar Absorption Lines" held in Shanghai, China from March 14th to 18th, 2005