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1-13 Constraints on Neutron Skin Thickness in 208Pb and Density-dependent Symmetry Energy 被引量:3

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摘要 Nuclear physics interacts with astrophysics, which not only expands its research space but also promotes the development of fundamental physics. Much attention has been paid to the equation of state (EOS) of isospin asymmetric nuclear matter as the development of radioactive beam facilities and astronomical observation facilities. The symmetry energy that measures the isospin-dependence of the EOS is a quantity of critical importance due to its many-sided roles. However, its density dependence remains a great challenge because of the incomplete knowledge of the nuclear force and the complexity of many-body systems. Many important issues in nuclear astrophysics urgently require accurate knowledge about it at present.
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出处 《IMP & HIRFL Annual Report》 2015年第1期21-21,共1页 中国科学院近代物理研究所和兰州重离子研究装置年报(英文版)
关键词 NEUTRON SKIN Thickness
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