Deconfinement phase Transition including perturbative QCD corrections in (proto)neutron star matter | |
Gu Jian-Fa2,4; Guo Hua1,2,4; Lee Xi-Guo1,3; Liu Yu-Xin1,2,4; Xu Fu-Rong1,2,4 | |
刊名 | COMMUNICATIONS IN THEORETICAL PHYSICS
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2008-02-01 | |
卷号 | 49期号:2页码:461-466 |
关键词 | deconfinement phase transition neutrino trapping neutron star matter |
ISSN号 | 0253-6102 |
英文摘要 | Deconfinement phase transition and neutrino trapping in (proto)neutron star matter are investigated in a chiral hadronic model (also referred to as the FST model) for the hadronic phase (HP) and in the color-flavor-locked (CFL) quark model for the deconfined quark phase. We include a perturbative QCD correction parameter alpha(s) in the CFL quark matter equation of states. It is shown that the CFL quark core with K-0 condensation forms in neutron star matter with the large value of alpha(s). If the small value of alpha(s) is taken, hyperons suppress the CFL quark phase and the HP is dominant in the high-density region of (proto)neutron star matter. Neutrino trapping makes the fraction of the CFL quark matter decrease compared with those without neutrino trapping. Moreover, increasing the QCD correction parameter alpha(s) or decreasing the bag constant B and the strange quark mass m(s) can make the fraction of the CFL quark matter increase, simultaneously, the fraction of neutrino in protoneutron star matter increases, too. The maximum masses and the corresponding radii of (proto)neutron stars are not sensitive to the QCD correction parameter alpha(s). |
WOS关键词 | GAUGE VECTOR-MESONS ; FINITE TEMPERATURE ; NEUTRON-STARS ; QUARK MATTER ; DENSITY ; NUCLEI ; FERMIONS ; ENERGY ; GAS |
WOS研究方向 | Physics |
语种 | 英语 |
出版者 | INT ACADEMIC PUBLISHERS LTD |
WOS记录号 | WOS:000253447100043 |
公开日期 | 2010-10-29 |
内容类型 | 期刊论文 |
源URL | [http://ir.imp.cas.cn/handle/113462/5795] ![]() |
专题 | 近代物理研究所_近代物理研究所知识存储(2010之前) |
通讯作者 | Gu Jian-Fa |
作者单位 | 1.Natl Lab Heavy Ion Accelerator, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China 2.Peking Univ, MOE Lab Heavy Ion Phys, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China 4.Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China |
推荐引用方式 GB/T 7714 | Gu Jian-Fa,Guo Hua,Lee Xi-Guo,et al. Deconfinement phase Transition including perturbative QCD corrections in (proto)neutron star matter[J]. COMMUNICATIONS IN THEORETICAL PHYSICS,2008,49(2):461-466. |
APA | Gu Jian-Fa,Guo Hua,Lee Xi-Guo,Liu Yu-Xin,&Xu Fu-Rong.(2008).Deconfinement phase Transition including perturbative QCD corrections in (proto)neutron star matter.COMMUNICATIONS IN THEORETICAL PHYSICS,49(2),461-466. |
MLA | Gu Jian-Fa,et al."Deconfinement phase Transition including perturbative QCD corrections in (proto)neutron star matter".COMMUNICATIONS IN THEORETICAL PHYSICS 49.2(2008):461-466. |
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