Post-Newtonian effects on the modes of rotating stars

Details Post-Newtonian effects on the modes of rotating stars Post-Newtonian effects on the modes of rotating stars

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...374..248c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 374, June 10, 1991, p. 248-254.

Statistics

Computation

18

Computational Astrophysics, Relativity, Stellar Oscillations, Stellar Rotation, Approximation, Stellar Gravitation

Scientific paper

A formidable unsolved problem in general relativity is how to calculate the nonaxisymmetric pulsational modes of rotating stars. Even in Newtonian gravity, the mode equations for rotating stars have only recently been solved numerically by Ipser and Lindblom (1989, 1990). In this paper, their Newtonian calculations are straightforwardly extended to post-Newtonian order.

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