A Family of Gravitational Waveforms from Rapidly Rotating Neutron Stars

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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TeX, 3 pages

Scientific paper

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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