Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2000-04-18
Phys.Rev. D62 (2000) 044006
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
13pages, no figures, accepted for publication in Physical Review D
Scientific paper
10.1103/PhysRevD.62.044006
Axial oscillations relevant to the r-mode instability are studied with slow rotation formalism in general relativity. The approximate equation governing the oscillations is derived with second-order rotational corrections. The equation contains an effective 'viscosity-like' term, which originates from coupling to the polar g-mode displacements. The term plays a crucial role on the resonance point, where the disturbance on the rotating stars satisfies a certain condition at the lowest order equation. The effect is significant for newly born hot neutron stars, which are expected to be subject to the gravitational radiation driven instability of the r-mode.
Hosonuma Masayasu
Kojima Yasufumi
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