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arXiv:1304.4007 [astro-ph.HE]AbstractReferencesReviewsResources

Compressed Baryonic Matter of Astrophysics

Yanjun Guo, Renxin Xu

Published 2013-04-15, updated 2013-07-22Version 2

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.

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
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