Extends FEW to produce adiabatic waveforms for eccentric equatorial inspirals into spinning black holes (|a|≤0.999) in ~100 ms with ~10^{-5} mismatches to reference waveforms.
Rel- ativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation,
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The Fast and the Frame-Dragging: Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly-spinning black holes
Extends FEW to produce adiabatic waveforms for eccentric equatorial inspirals into spinning black holes (|a|≤0.999) in ~100 ms with ~10^{-5} mismatches to reference waveforms.