A new method for treating nonradial pulsations in general relativity

Astronomy and Astrophysics – Astronomy

Scientific paper

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Equations Of Motion, Newton Theory, Relativity, Stellar Models, Stellar Oscillations, Boundary Conditions, Gravitational Waves, Stellar Rotation

Scientific paper

It is described how Newtonian techniques for rapidly rotating inhomogeneous stellar models can be extended to a treatment of nonradial perturbations of spherical stellar models in general relativity. Problems discussed include the perturbation equations for a nonradial mode, reduction to an explicitly fourth-order system inside the stellar model, a second-order equation for K in the exterior vacuum, and boundary conditions.

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