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作 者:WANG HongYan LIU GuangZhou WU YaoRui XU Yan ZHU MingFeng BAO Tmurbagan
机构地区:[1]College of Physics, Jilin University [2]College of Physics, Beihua University [3]College of Computer Science and Technology, Jilin University [4]Changchun Observatory,National Astronomical Observatories, Chinese Academy of Sciences [5]Institute for Numerical Calculations, College of Physics and Electronic Information, Inner Mongolia University for the Nationalities
出 处:《Chinese Science Bulletin》2013年第31期3731-3734,共4页
基 金:supported by the National Natural Science Foundation of China(10675024,11075063,11265009);National Fund for Fostering Talents of Basic Science (J1103202)
摘 要:In this paper,we study the third family of compact stars with the color-flavor locked(CFL)quark core.The relativistic mean field model is used for hadronic matter and the MIT bag model for CFL quark matter.The results of the calculation show a transitional behavior that goes from the hadron star range,through the transition range,into the CFL quark star range.In the transition range,the third family of compact stars with the CFL quark matter core is found in the wide range of the CFL energy gap 100MeV≤<150 MeV.By comparing with early investigations,we argue that the greatest possible third family of compact stars may be the hybrid stars with the CFL quark core.In this paper, we study the third family of compact stars with the color-flavor locked (CFL) quark core. The relativistic mean field model is used for hadronic matter and the MIT bag model for CFL quark matter. The results of the calculation show a transitional behavior that goes from the hadron star range, through the transition range, into the CFL quark star range. In the transition range, the third family of compact stars with the CFL quark matter core is found in the wide range of the CFL energy gap 100 MeV~〈A〈150 MeV. By comparing with early investigations, we argue that the greatest possible third family of compact stars may be the hybrid stars with the CFL quark core.
关 键 词:紧凑型荧光灯 夸克物质 锁定 同色 相对论平均场模型 家族 恒星 CFL
分 类 号:O572.33[理学—粒子物理与原子核物理]
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