Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars

  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},
Associated Articles Part  1     Part  2     Part  3     Part  5     Part  7     Part  4     Part  8     Part  6 
Models of Rotating Neutron Stars in General Relativity
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.
Particle acceleration and electromagnetic field of deformed neutron stars
Neutron stars (NS)s are astrophysical objects with strong gravitational and electromagnetic fields. Since there are several effects on radiation processes around the star, it is impossible to consi...
Rotating neutron stars in a chiral SU(3) model
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Neutron-star models in Ni's theory of gravity
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Rotational Deformation of Neutron Stars
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
Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field
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
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
General Relativistic Theory of Rotating Neutron Stars — A Review
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