Slowly Rotating Relativistic Stars. I. Equations of Structure
@article{Hartle1967SlowlyRR, title={Slowly Rotating Relativistic Stars. I. Equations of Structure}, author={James B. Hartle}, journal={The Astrophysical Journal}, year={1967}, volume={150}, pages={1005-1029} }
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586 Citations
Rotating relativistic stars: two problems
- Physics, Mathematics
- 2005
In this article we discuss two problems related to rotating stars. The first part of the article deals a recent suggestion [11] that w-modes of supercompact stars might become CFS unstable, while in…
Evolution equations for slowly rotating stars
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- 2005
We present a hyperbolic formulation of the evolution equations describing nonradial perturbations of slowly rotating relativistic stars in the Regge–Wheeler gauge. We demonstrate the stability…
Post-Minkowskian analysis of slowly rotating stars
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The formalism developed by Hartle is used to set up the fieldequations of slowly and rigidly rotating stars valid to secondorder in the rotation parameter. These equations are then solvedin the ext…
Torsional Oscillations of Slowly Rotating Relativistic Stars
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- 2007
We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional…
Torsional oscillations of slowly rotating relativistic stars
- Physics
- 2007
We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional…
WARM STELLAR MATTER: APPLICATION TO SLOWLY ROTATING COMPACT OBJECTS
- Physics
- 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…
Envelopes of rapidly rotating neutron stars
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- 1985
Motivated by the discovery of the millisecond pulsars, we consider the effect of rapid rotation on the envelope of a neutron star. Solving the equation of hydrostatic equilibrium we find expressions…
Analytic neutron stars in general relativity: Exact solutions for the non-homogeneous charged model
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We have extended the so-called Adams' method to the non-homogeneous charged model of neutron stars. Numerical applications have been compared with results obtained for a given equation of state.
Rotating white dwarfs in the general relativity theory
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Translated from Astrofizika; 7: No. 3, 467-479(1971) . The principal integral characteristics of rotating white dwarfs are presented which have been calculated in the OMEGA /sup 2/ approximation (…