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.
Black hole perturbation theory and gravitational self-force,
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 2years
2025 2roles
background 1polarities
background 1representative 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
-
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.
-
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.