Frontiers the Physics of Dense Matter for Neutron Stars

被引：1
|
作者：
Steiner, Andrew W. [1 ,2 ]
机构：
[1] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[2] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
来源：
XIII INTERNATIONAL WORKSHOP ON HADRON PHYSICS, SECTIONS 1-5 | 2016年 / 706卷
关键词：
EQUATION-OF-STATE; MASSES; RADII; NUCLEI;
D O I：
10.1088/1742-6596/706/2/022001
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Neutron stars are an excellent laboratory for nuclear physics. They probe the nucleon-nucleon interaction, the structure of nuclei, and the nature of dense QCD in ways which complement current experimental efforts. This article very briefly summarizes some of the current frontiers in neutron stars and dense matter with an emphasis on how our understanding might be improved in the near future.
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页数：10
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