%0 Journal Article
%T A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars
%A Dong Lai
%J Physics
%D 1999
%I arXiv
%X 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.
%U http://arxiv.org/abs/gr-qc/9902068v1