A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars
classification
🌀 gr-qc
keywords
gravitationalneutronrapidlyrotatingwaveformsaxisymmetriccollapseconfiguration
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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.
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