Density-dependent symmetry energy at subsaturation densities from nuclear mass differences

被引:27
作者
Fan, Xiaohua [1 ,2 ]
Dong, Jianmin [1 ,3 ]
Zuo, Wei [1 ]
机构
[1] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
[2] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[3] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
来源
PHYSICAL REVIEW C | 2014年 / 89卷 / 01期
基金
中国国家自然科学基金;
关键词
NEUTRON-STAR; EQUATION; RADII;
D O I
10.1103/PhysRevC.89.017305
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We extract the mass-dependent symmetry energy coefficients a(sym)(A) with the nuclear mass differences reducing the uncertainties as far as possible. The estimated asym(A) of Pb-208 is 22.4 +/- 0.3 MeV, which is further used to analyze the density-dependent nuclear matter symmetry energy at subsaturation densities. The slope parameter of the symmetry energy at the saturation density rho(0) is L = 50.0 +/- 15.5 MeV. Furthermore, it is found that at the density of rho = 0.69 rho(0) = 0.11 fm(-3), the symmetry energy S(rho = 0.11 fm(-3)) = 25.98 +/- 0.01 MeV and the corresponding slope parameter is L = 49.6 +/- 6.2 MeV, which are consistent with other independent analyses.
引用
收藏
页数:4
相关论文
共 38 条
  • [1] Constraining the density dependence of the symmetry energy from nuclear masses
    Agrawal, B. K.
    De, J. N.
    Samaddar, S. K.
    Colo, G.
    Sulaksono, A.
    [J]. PHYSICAL REVIEW C, 2013, 87 (05):
  • [2] Determining the Density Content of Symmetry Energy and Neutron Skin: An Empirical Approach
    Agrawal, B. K.
    De, J. N.
    Samaddar, S. K.
    [J]. PHYSICAL REVIEW LETTERS, 2012, 109 (26)
  • [3] Reaction dynamics with exotic nuclei
    Baran, V
    Colonna, M
    Greco, V
    Di Toro, M
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2005, 410 (5-6): : 335 - 466
  • [4] Neutron radii in nuclei and the neutron equation of state
    Brown, BA
    [J]. PHYSICAL REVIEW LETTERS, 2000, 85 (25) : 5296 - 5299
  • [5] Constraints on the symmetry energy and neutron skins from pygmy resonances in 68Ni and 132Sn
    Carbone, Andrea
    Colo, Gianluca
    Bracco, Angela
    Cao, Li-Gang
    Bortignon, Pier Francesco
    Camera, Franco
    Wieland, Oliver
    [J]. PHYSICAL REVIEW C, 2010, 81 (04):
  • [6] Nuclear Symmetry Energy Probed by Neutron Skin Thickness of Nuclei
    Centelles, M.
    Roca-Maza, X.
    Vinas, X.
    Warda, M.
    [J]. PHYSICAL REVIEW LETTERS, 2009, 102 (12)
  • [7] Surface symmetry energy
    Danielewicz, P
    [J]. NUCLEAR PHYSICS A, 2003, 727 (3-4) : 233 - 268
  • [8] Symmetry energy I: Semi-infinite matter
    Danielewicz, Pawel
    Lee, Jenny
    [J]. NUCLEAR PHYSICS A, 2009, 818 (1-2) : 36 - 96
  • [9] Density dependence of the symmetry energy probed by β- decay energies of odd-A nuclei
    Dong, Jianmin
    Zhang, Haifei
    Wang, Longjun
    Zuo, Wei
    [J]. PHYSICAL REVIEW C, 2013, 88 (01):
  • [10] Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured α-decay energies
    Dong, Jianmin
    Zuo, Wei
    Gu, Jianzhong
    [J]. PHYSICAL REVIEW C, 2013, 87 (01):