How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas?
equation of state、symmetry energy、asymmetric nuclear matter、order parameters
28
O4 ;O57
NBZ is supported in part by the China Scholarship Council. BAL acknowledges the U.S. Department of Energy, Office of Science, under Award Number DE-SC0013702, the CUSTIPEN China-U.S. Theory Institute for Physics with Exotic Nuclei under the US Department of Energy Grant No. DE-SC0009971, the National Natural Science Foundation of China under Grant No. 11320101004 and the Texas Advanced Computing Center. JX is supported in part by the Major State Basic Research Development Program 973 Program of China under Contract Nos. 2015CB856904 and 2014CB845401, the National Natural Science Foundation of China under Grant Nos. 11475243 and 11421505, the”100-talent plan” of Shanghai Institute of Applied Physics under Grant Nos. Y290061011 and Y526011011 from the Chinese Academy of Sciences, the Shanghai Key Laboratory of Particle Physics and Cosmology under Grant No. 15DZ2272100, and the Shanghai Pujiang Program under Grant No. 13PJ1410600
2018-01-10(万方平台首次上网日期,不代表论文的发表时间)
共7页
79-85