The nuclear physics of neutron stars

被引:0
|
作者
Piekarewicz, J. [1 ]
机构
[1] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA
关键词
Nuclear matter; neutron stars; effective interactions;
D O I
暂无
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A remarkable fact about spherically-symmetric neutron stars in hydrostatic equilibrium - the so-called Schwarzschild stars - is that the only physics that they are sensitive to is the equation of state of neutron-rich matter. As such, neutron stars provide a myriad of observables that may be used to constrain poorly known aspects of the nuclear interaction under extreme conditions of density. After discussing many of the fascinating phases encountered in neutron stars, I will address how powerful theoretical, experimental, and observational constraints may be used to place stringent limits on the equation of state of neutron-rich matter.
引用
收藏
页码:104 / 109
页数:6
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