Gravitational-wave driven instability of rotating relativistic stars

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dc.creatorFriedman, John L.
dc.creatorLockitch, Keith H.
dc.date1999-08-31
dc.date.accessioned2026-07-07T11:08:47Z
dc.date.available2026-07-07T11:08:47Z
dc.descriptionA 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.
dc.description14 pages PTPTeX v.1.0. Contribution to proceedings of the 1999 Yukawa International Seminar
dc.identifierhttps://arxiv.org/abs/gr-qc/9908083
dc.identifierhttp://arxiv.org/abs/gr-qc/9908083
dc.identifierProg.Theor.Phys.Suppl.136:121-134,1999
dc.identifierdoi:10.1143/PTPS.136.121
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190255
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleGravitational-wave driven instability of rotating relativistic stars
dc.typetext

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