The nonadiabatic general-relativistic stellar oscillations

Details The nonadiabatic general-relativistic stellar oscillations The nonadiabatic general-relativistic stellar oscillations

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.168..305m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 168, no. 2, June 1990, p. 305-316. Research supported by CICYT and Consell

Statistics

Computation

Neutron Stars, Relativistic Effects, Stellar Oscillations, Computational Astrophysics, Einstein Equations, Perturbation Theory, Stellar Models

Scientific paper

This paper derives 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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