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20 April 2024

» arxiv » gr-qc/9902068

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A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars
Dong Lai ;
Date:	22 Feb 1999
Subject:	gr-qc
Affiliation:	Cornell
Abstract:	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.
Source:	arXiv, gr-qc/9902068
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