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The nonadiabatic general-relativistic stellar oscillations
Authors:José Ma. Martí  Juan A. Miralles  José Ma. Ibánez  Luis Herrera
Affiliation:(1) Departamento de Física Teórica, Universidad de Valencia, Burjassot, Valencia, Spain;(2) Departamento de Física, Facultad de Ciencias, Universidad de las Islas Baleares, Palma de Mallorca, Spain
Abstract:We have derived the equations which govern the linear nonadiabatic general-relativistic radial oscillations. The perturbation produces a heat flux that is coupled with the geometry, through the Einstein field equations of a stellar configuration. The classical limit is recovered. The stability conditions are examined by means of a simplified one-zone model.
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