Constraining the equation of state with moment of inertia measurements

被引:336
作者
Lattimer, JM [1 ]
Schutz, BF
机构
[1] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[2] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Potsdam, Germany
关键词
binaries : close; equation of state; pulsars : general;
D O I
10.1086/431543
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We estimate that the moment of inertia of star A in the recently discovered double pulsar system PSR J0737 - 3039 may be determined after a few years of observation to similar to 10% accuracy. This would enable accurate estimates of the radius of the star and the pressure of matter in the vicinity of 1 - 2 times the nuclear saturation density, which would in turn provide strong constraints on the equation of state of neutron stars and the physics of their interiors.
引用
收藏
页码:979 / 984
页数:6
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