Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars
@article{Hartle1968SlowlyRR, title={Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars}, author={James B. Hartle and Kip S. Thorne}, journal={The Astrophysical Journal}, year={1968}, volume={153}, pages={807} }
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492 Citations
Models of Rotating Neutron Stars in General Relativity
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We describe a numerical method of integration of Einstein’s equations coupled with the hydrodynamic equations for a perfect fluid. We give, also, some preliminary results.
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The rotational deformations of two kinds of neutron stars are calculated by using Hartle's slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious…
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- 2007
Properties and deformations of the rotating neutron stars in uniform strong magnetic field are calculated. The magnetic field will soften the equation of state of the neutron star matters and make an…
WARM STELLAR MATTER: APPLICATION TO SLOWLY ROTATING COMPACT OBJECTS
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- 2008
In the present paper we investigate one possible variation on the usual static pulsars: the inclusion of rotation. We use a formalism proposed by Hartle and Thorne to calculate the properties of…
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Except in cosmology, astrophysicists are used to thinking of general relativistic effects as small (e.g., light bending, perihelion advance, red shift) and have generally left such problems to…