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arXiv · gr-qc/9908083

Gravitational-wave driven instability of rotating relativistic stars

John L. Friedman·Keith H. Lockitch
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Abstract

A brief review of the stability of rotating relativistic stars is followed by a more detailed discussion of recent work on an instability of r-modes, modes of rotating stars that have axial parity in the slow-rotation limit. These modes may dominate the spin-down of neutron stars that are rapidly rotating at birth, and the gravitational waves they emit may be detectable.

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John L. Friedman, Keith H. Lockitch. 1999-08-31. Gravitational-wave driven instability of rotating relativistic stars. https://doi.org/10.1143/ptps.136.121

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