Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars

	Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars
其他题名	论文其他题名
	Bao T. B.; Liu G. Z.; Zhu M. F.
	2006
发表期刊	High Energy Physics and Nuclear Physics-Chinese Edition
ISSN	0254-3052
卷号	30 页码:255-257
摘要	Upon application of the mass-density-dependent quark model with thermodynamic self-consistency, we investigate the bulk properties of hybrid stars and calculate the particle fraction and equation of state(EOS) for hybrid star matter. Numerical results indicate that the pressure extra term deriving from self-consistently thermodynamical treatment can soften the EOS, put off the appearence of phase transition and decrease the maximum mass for a hybrid star from 2.4(circle dot) (without pressure extra term) to 1.8M(circle dot) with corresponding radius from 15km to 12km. Similar to the Nambu-Jona-Lasinio(NJL) model, this model is suitable for describing the massive hybrid stars.
收录类别	SCI
语种	中文
文献类型	期刊论文
条目标识符	http://ir.ciomp.ac.cn/handle/181722/25731
专题	中科院长春光机所知识产出
推荐引用方式 GB/T 7714	Bao T. B.,Liu G. Z.,Zhu M. F.. Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars[J]. High Energy Physics and Nuclear Physics-Chinese Edition,2006,30:255-257.
APA	Bao T. B.,Liu G. Z.,&Zhu M. F..(2006).Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars.High Energy Physics and Nuclear Physics-Chinese Edition,30,255-257.
MLA	Bao T. B.,et al."Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars".High Energy Physics and Nuclear Physics-Chinese Edition 30(2006):255-257.

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