Relativistic Calculation of r-MODE Oscillations Without Metric Perturbations

Physics

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Scientific paper

The axial mode oscillations are examined for relativistic rotating stars with uniform angular velocity. Using the slow rotation formalism, the rotational corrections up to the second order are included to the oscillation equations. The equations governing the r-mode oscillations are derived, neglecting the metric perturbations, i.e. in the Cowling approximation.

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