activity
20102020
most citedExtreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole

100 citations · 202 across the 3 of their papers we have counts for

collaborators

5 papers

gr-qc202081 cited

Adding Gravitational Memory to Waveform Catalogs using BMS Balance Laws

Keefe Mitman, Dante A. B. Iozzo, Neev Khera +9

Accurate models of gravitational waves from merging binary black holes are crucial for detectors to measure events and extract new science. One important feature that is currently…

gr-qc202021 cited

High-accuracy waveforms for black hole-neutron star systems with spinning black holes

Francois Foucart, Alexander Chernoglazov, Michael Boyle +10

The availability of accurate numerical waveforms is an important requirement for the creation and calibration of reliable waveform models for gravitational wave astrophysics. For b…

gr-qc2020

Computation of Displacement and Spin Gravitational Memory in Numerical Relativity

Keefe Mitman, Jordan Moxon, Mark A. Scheel +5

We present the first numerical relativity waveforms for binary black hole mergers produced using spectral methods that show both the displacement and the spin memory effects. Expli…

math.NA2018

A high-order, conservative integrator with local time-stepping

William Throwe, Saul A. Teukolsky

We present a family of multistep integrators based on the Adams-Bashforth methods. These schemes can be constructed for arbitrary convergence order with arbitrary step size variati…

gr-qc2010100 cited

Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole

Nicolas Yunes, Alessandra Buonanno, Scott A. Hughes +4

We construct effective-one-body waveform models suitable for data analysis with LISA for extreme-mass ratio inspirals in quasi-circular, equatorial orbits about a spinning supermas…