A Model Study of Equation of State of QCD at Finite Chemical Potential and Zero Temperature

被引:0
|
作者
Hou Feng-Yao [1 ,2 ]
Jiang Yu [1 ]
Sun Wei-Min [1 ,3 ]
Zong Hong-Shi [1 ,3 ]
机构
[1] Nanjing Univ, Dept Phys, Nanjing 210093, Peoples R China
[2] Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China
[3] Joint Ctr Particle Nucl Phys & Cosmol, Nanjing 210093, Peoples R China
关键词
equation of state (EOS); phase transition; QCD; CHIRAL-SYMMETRY RESTORATION; DYSON-SCHWINGER EQUATIONS; SELF-ENERGY;
D O I
暂无
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper, we give a direct method for calculating the partition function, and hence the equation of state (EOS) of QCD at finite chemical potential and zero temperature. In the EOS derived in this paper the pressure density is the sum of two terms: the first term P(mu)vertical bar(mu=0) (the pressure density at mu = 0) is a mu-independent constant; the second term, which is totally determined by G[mu](p) (the dressed quark propagator at finite mu), contains all the nontrivial mu-dependence. By applying a general result in the rainbow-ladder approximation of the Dyson-Schwiner approach obtained in our previous study [Phys. Rev. C 71 (2005) 015205], G[mu](p) is calculated from the meromorphic quark propagator proposed in [Phys. Rev. D 67 (2003) 054019]. From this the full analytic expression of the EOS of QCD at finite mu and zero T is obtained (apart from the constant term P(mu)vertical bar(mu=0), which can be principle be calculated from the CJT effective action). A comparison between our EOS and the cold, perturbative EOS of QCD of Fraga, Pisarski and Schaffner-Bielich is made. It is expected that our EOS can provide a possible new approach for the study of neutron stars.
引用
收藏
页码:499 / 505
页数:7
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