Non-Radial Oscillations of Stars in General Relativity: A Scattering Problem

Details Non-Radial Oscillations of Stars in General Relativity: A Scattering Problem Non-Radial Oscillations of Stars in General Relativity: A Scattering Problem

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rspta.340..423f&link_type=abstract

Philosophical Transactions: Physical Sciences and Engineering, Volume 340, Issue 1658, pp. 423-445

Physics

7

Scientific paper

The problem of non-radial oscillations of stars can be formulated as a problem of resonant scattering of gravitational waves incident on the potential barrier generated by the space-time curvature. This approach discloses some unexpected correspondences between the theory of perturbations of stars and the theory of quantum mechanics. New relativistic effects are predicted, as the resonant behaviour of the axial modes in slowly rotating stars, due to the coupling with the polar modes induced by the Lense-Thirring effect.

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