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Nuclear matter symmetry energy and the symmetry energy coefficient in the mass formula

Journal Article · · Physical Review. C, Nuclear Physics
 [1]
  1. Department of Physics, Shanghai Jiao Tong University, Shanghai 200240 (China) and Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000 (China)
Within the Skyrme-Hartree-Fock (SHF) approach, we show that for a fixed mass number A, both the symmetry energy coefficient a{sub sym}(A) in the semiempirical mass formula and the nuclear matter symmetry energy E{sub sym}({rho}{sub A}) at a subsaturation reference density {rho}{sub A} can be determined essentially by the symmetry energy E{sub sym}({rho}{sub 0}) and its density slope L at saturation density {rho}{sub 0}. Meanwhile, we find the dependence of a{sub sym}(A) on E{sub sym}({rho}{sub 0}) or L is approximately linear and very similar to the corresponding linear dependence displayed by E{sub sym}({rho}{sub A}), providing an explanation for the relation E{sub sym}({rho}{sub A}){approx_equal}a{sub sym}(A).Our results indicate that a value of E{sub sym}({rho}{sub A}) leads to a linear correlation between E{sub sym}({rho}{sub 0}) and L and thus can put important constraints on E{sub sym}({rho}{sub 0}) and L. Particularly, the values of E{sub sym}({rho}{sub 0})=30.5{+-}3 MeV and L= 52.5{+-}20 MeV are simultaneously obtained by combining the constraints from recently extracted E{sub sym}({rho}{sub A}=0.1 fm{sup -3}) with those from recent analyses of neutron skin thickness of Sn isotopes in the same SHF approach.
OSTI ID:
21499559
Journal Information:
Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 4 Vol. 83; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English