A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars

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This 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.
TeX, 3 pages

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/36446

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/9902068
 http://arxiv.org/abs/gr-qc/9902068

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arXiv