CONSTRAINING THE SYMMETRY ENERGY FROM THE NEUTRON SKIN THICKNESS OF TIN ISOTOPES
We show in the Skyrme-Hartree-Fock approach that unambiguous correlations exist between observables of finite nuclei and nuclear matter properties. Using this correlation analysis to existing data on the neutron skin thickness of Sn isotopes, we find important constraints on the value Eaym(po) and density slope L of the nuclear symmetry energy at saturation density. Combining these constraints with those from recent analyses of isospin diffusion and double neutron/proton ratio in heavy ion collisions leads to a value of L = 58 ± 18 MeV approximately independent of Eaym(po).
Nuclear symmetry energy neutron skin Skyrme Hartree-Fock
LIE-WEN CHEN CHE MING KO JUN XU BAO-AN LI
Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Department of Physics and Astronomy, Texas A&M University-Commerce, Commerce, Texas 75429-3011, USA
国际会议
The 13th National Conference on Nuclear Structure(第十三届全国核结构研讨会暨第九次全国“核结构与量子力学专题讨论会
赤峰
英文
15-20
2010-07-24(万方平台首次上网日期,不代表论文的发表时间)