A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars
arXiv:gr-qc/9902068
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.
TeX, 3 pages