activity
19942026
most citedAn improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors

615 citations · 18k across the 232 of their papers we have counts for

collaborators
Showing 2011 · gr-qcShow all

5 papers · 2 filters

gr-qc2011★ 69 cited

Black hole-neutron star mergers for 10 solar mass black holes

Francois Foucart, Matthew D. Duez, Lawrence E. Kidder +3

General relativistic simulations of black hole-neutron star mergers have currently been limited to low-mass black holes (less than 7 solar mass), even though population synthesis m…

gr-qc2011★ 97 cited

Accurate gravitational waveforms for binary-black-hole mergers with nearly extremal spins

Geoffrey Lovelace, Michael Boyle, Mark A. Scheel +1

Motivated by the possibility of observing gravitational waves from merging black holes whose spins are nearly extremal (i.e., 1 in dimensionless units), we present numerical wavefo…

gr-qc2011★ 17 cited

On Toroidal Horizons in Binary Black Hole Inspirals

Michael I. Cohen, Jeffrey D. Kaplan, Mark A. Scheel

We examine the structure of the event horizon for numerical simulations of two black holes that begin in a quasicircular orbit, inspiral, and finally merge. We find that the spatia…

gr-qc2011★ 79 cited

Visualizing Spacetime Curvature via Frame-Drag Vortexes and Tidal Tendexes I. General Theory and Weak-Gravity Applications

David A. Nichols, Robert Owen, Fan Zhang +8

When one splits spacetime into space plus time, the Weyl curvature tensor (vacuum Riemann tensor) gets split into two spatial, symmetric, and trace-free (STF) tensors: (i) the Weyl…

gr-qc2011★ 261 cited

Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism

Yi Pan, Alessandra Buonanno, Michael Boyle +4

We calibrate an effective-one-body (EOB) model to numerical-relativity simulations of mass ratios 1, 2, 3, 4, and 6, by maximizing phase and amplitude agreement of the leading (2,2…