A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars

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dc.creatorLai, Dong
dc.date1999-02-22
dc.date.accessioned2026-07-07T03:32:59Z
dc.date.available2026-07-07T03:32:59Z
dc.descriptionThis note describes fitting formulae for the gravitational waveforms generated by a rapidly rotating neutron star (e.g., newly-formed in the core collapse of a supernova) as it evolves from an initial axisymmetric configuration toward a triaxial ellipsoid.
dc.descriptionTeX, 3 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9902068
dc.identifierhttp://arxiv.org/abs/gr-qc/9902068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36446
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars
dc.typetext

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