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.
Transition from Inspiral to Plunge: A Complete Near-Extremal Tra- jectory and Associated Waveform
2 Pith papers cite this work. Polarity classification is still indexing.
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gr-qc 2years
2025 2representative citing papers
For high-spin Kerr circular orbits, l_max >=30 and Chebyshev interpolation with global relative flux error matching the mass ratio yield mismatches below 10^{-3} and negligible parameter biases in 4-year EMRI signals with SNR ~100.
citing papers explorer
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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.
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Systematic errors in fast relativistic waveforms for Extreme Mass Ratio Inspirals
For high-spin Kerr circular orbits, l_max >=30 and Chebyshev interpolation with global relative flux error matching the mass ratio yield mismatches below 10^{-3} and negligible parameter biases in 4-year EMRI signals with SNR ~100.