中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Deconfinement phase transition in neutron star matter

文献类型:期刊论文

作者Li, A; Peng GX(彭光雄); Peng, GX; Lombardo, U
刊名CHINESE PHYSICS C
出版日期2009
卷号33页码:#REF!
关键词phase transition the density-dependent quark model three-body force
通讯作者Li, A (reprint author), Xiamen Univ, Dept Phys, Xiamen 361005, Peoples R China.
英文摘要The transition from hadron phase to strange quark phase in dense matter is investigated. Instead of using the conventional bag model in quark sect, we achieve the confinement by a density-dependent quark mass derived from in-medium chiral condensates, with a thermodynamic problem improved. In nuclear slot, we adopt the equation of state from Brueckner-Bethe-Goldstone approach with three-body force. It is found that the mixed phase can occur, for reasonable confinement, parameter, near the normal saturation density, and transit to pure quark matter at 4-5 times the saturation, which is quite different from the previous results from other quark models that pure quark phase can not appear at neutron-star densities.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
收录类别SCI
WOS记录号WOS:000264986200020
公开日期2016-05-03
源URL[http://ir.ihep.ac.cn/handle/311005/225845]  
专题高能物理研究所_理论物理室
推荐引用方式
GB/T 7714
Li, A,Peng GX,Peng, GX,et al. Deconfinement phase transition in neutron star matter[J]. CHINESE PHYSICS C,2009,33:#REF!.
APA Li, A,彭光雄,Peng, GX,&Lombardo, U.(2009).Deconfinement phase transition in neutron star matter.CHINESE PHYSICS C,33,#REF!.
MLA Li, A,et al."Deconfinement phase transition in neutron star matter".CHINESE PHYSICS C 33(2009):#REF!.

入库方式: OAI收割

来源:高能物理研究所

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