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6 papers · 2 filters
Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
E. A. Huerta, C. J. Moore, Prayush Kumar +10
We present , a time domain, inspiral-merger-ringdown waveform model that describes non-spinning binary black holes systems that evolve on moderately eccentric orbi…
Systematic challenges for future gravitational wave measurements of precessing binary black holes
A. R. Williamson, J. Lange, R. O'Shaughnessy +4
The properties of precessing, coalescing binary black holes are presently inferred through comparison with two approximate models of compact binary coalescence. In this work we sho…
Scalar, Vector and Tensor Harmonics on the Three-Sphere
Lee Lindblom, Nicholas W. Taylor, Fan Zhang
Scalar, vector and tensor harmonics on the three-sphere were introduced originally to facilitate the study of various problems in gravitational physics. These harmonics are defined…
Stability of stationary-axisymmetric black holes in vacuum general relativity to axisymmetric electromagnetic perturbations
Kartik Prabhu, Robert M. Wald
We consider arbitrary stationary and axisymmetric black holes in general relativity in dimensions (with ) that satisfy the vacuum Einstein equation and have a no…
Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription
Chris Kavanagh, Donato Bini, Thibault Damour +3
In this work we present an analytical gravitational self-force calculation of the spin-orbit precession along an eccentric orbit around a Schwarzschild black hole, following closel…
A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
Jacob Lange, Richard O'Shaughnessy, Michael Boyle +23
We present and assess a Bayesian method to interpret gravitational wave signals from binary black holes. Our method directly compares gravitational wave data to numerical relativit…