NTUEENTUEE 1 Introduction to Cadence 講員:張祐齊 日期: 2002.02.27 原講員:魏睿民 1999.10.08.
Compact Stars With a Dyson- Schwinger Quark Model 1 陈 欢 Collaborate with 魏金标( CUG ),...
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Structure of Compact stars 3 CUG, Wuhan, China 1. A compact star with 2 solar-mass could reach a baryon number density about 1fm -3, quark would become an active degree of freedom, e.g. quark deconfinemt. 2. Possible strange quark stars with stable strange quark matter hypothesis. F.Weber, et.al. astro-ph/ H. Chen Xiamen