期刊
ASTROPHYSICAL JOURNAL
卷 629, 期 2, 页码 979-984出版社
UNIV CHICAGO PRESS
DOI: 10.1086/431543
关键词
binaries : close; equation of state; pulsars : general
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.
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