Compressed Baryonic Matter of Astrophysics
High Energy Astrophysical Phenomena
2013-07-23 v2 Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
Nuclear Theory
Abstract
Baryonic matter in the core of a massive and evolved star is compressed significantly to form a supra-nuclear object, and compressed baryonic matter (CBM) is then produced after supernova. The state of cold matter at a few nuclear density is pedagogically reviewed, with significant attention paid to a possible quark-cluster state conjectured from an astrophysical point of view.
Keywords
Cite
@article{arxiv.1304.4007,
title = {Compressed Baryonic Matter of Astrophysics},
author = {Yanjun Guo and Renxin Xu},
journal= {arXiv preprint arXiv:1304.4007},
year = {2013}
}
Comments
10 pages, Contribution for the Conference Proceedings of the Compact Stars in the QCD Phase Diagram III (CSQCD III), December 12-15, 2012, Guaruj\'a, Brazil. http://www.astro.iag.usp.br/~foton/CSQCD3