Liquid-gas phase transition in hot asymmetric nuclear matter with density-dependent relativistic mean-field models

被引:19
作者
Zhang, Guang-Hua [1 ]
Jiang, Wei-Zhou [1 ,2 ]
机构
[1] Southeast Univ, Dept Phys, Nanjing 211189, Jiangsu, Peoples R China
[2] Natl Lab Heavy Ion Accelerator, Lanzhou 730000, Peoples R China
基金
中国国家自然科学基金;
关键词
ISOSPIN; FRAGMENTATION; EQUATION; STATE; WARM;
D O I
10.1016/j.physletb.2013.01.066
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The liquid-gas phase transition in hot asymmetric nuclear matter is studied within density-dependent relativistic mean-field models where the density dependence is introduced according to the Brown-Rho scaling and constrained by available data at low densities and empirical properties of nuclear matter. The critical temperature of the liquid-gas phase transition is obtained to be 15.7 MeV in symmetric nuclear matter falling on the lower edge of the small experimental error bars. In hot asymmetric matter, the boundary of the phase-coexistence region is found to be sensitive to the density dependence of the symmetry energy. The critical pressure and the area of phase-coexistence region increases clearly with the softening of the symmetry energy. The critical temperature of hot asymmetric matter separating the single-phase region from the two-phase region is analyzed to have a moderate sensitivity to the symmetry energy and is higher for the model possessing the softer symmetry energy. Crown Copyright (C) 2013 Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:148 / 152
页数:5
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