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作 者:WANG Ning LIU Min WU Xi-zhen
机构地区:[1]Department of Physics, Guangxi Normal University, Guilin
出 处:《Annual Report of China Institute of Atomic Energy》2010年第1期81-82,共2页中国原子能科学研究院年报(英文版)
基 金:Supported by National Natural Science Foundation of China
摘 要:The nuclear mass is of great importance not only for various aspects of nuclear physics, but also for weak-interaction studies and astrophysics. In the nuclear physics, it is helpful to study the nuclear symmetry energy and the synthesis of superheavy nuclei by considering the more than 2 000The nuclear mass is of great importance not only for various aspects of nuclear physics, but also for weak-interaction studies and astrophysics. In the nuclear physics, it is helpful to study the nuclear symmetry energy and the synthesis of superheavy nuclei by considering the more than 2 000 measured nuclear masses. Theoretically, the mass of an atomic nucleus can be calculated by the macroscopic- microscopic method (such as the finite-range droplet model) or the microscopic approaches (such as Hartree-Fock Bogoliubov approach) or some other mass formulas. The best mass formulas at present can reach about 0.6 MeV in the rms deviation for the usual data set of 2 149 measured masses of nuclei with about 24-30 model parameters.
关 键 词:质量公式 同位旋效应 HARTREE-FOCK 修改 弱相互作用 超重核合成 均方根误差 天体物理
分 类 号:O571.6[理学—粒子物理与原子核物理] P145.8[理学—物理]
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