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20002024
most citedThe PyCBC search for gravitational waves from compact binary coalescence

649 citations · 15.5k across the 171 of their papers we have counts for

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Showing 2008Show all

8 papers · 1 filter

gr-qc2008★ 51 cited

Implementation of higher-order absorbing boundary conditions for the Einstein equations

Oliver Rinne, Luisa T. Buchman, Mark A. Scheel +1

We present an implementation of absorbing boundary conditions for the Einstein equations based on the recent work of Buchman and Sarbach. In this paper, we assume that spacetime ma…

gr-qc2008★ 296 cited

High-accuracy waveforms for binary black hole inspiral, merger, and ringdown

Mark A. Scheel, Michael Boyle, Tony Chu +3

The first spectral numerical simulations of 16 orbits, merger, and ringdown of an equal-mass non-spinning binary black hole system are presented. Gravitational waveforms from these…

gr-qc2008★ 173 cited

Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods

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

We present a code for solving the coupled Einstein-hydrodynamics equations to evolve relativistic, self-gravitating fluids. The Einstein field equations are solved in generalized h…

gr-qc2008★ 25 cited

Revisiting Event Horizon Finders

Michael I. Cohen, Harald P. Pfeiffer, Mark A. Scheel

Event horizons are the defining physical features of black hole spacetimes, and are of considerable interest in studying black hole dynamics. Here, we reconsider three techniques t…

gr-qc2008★ 12 cited

IMEX evolution of scalar fields on curved backgrounds

Stephen R. Lau, Harald P. Pfeiffer, Jan S. Hesthaven

Inspiral of binary black holes occurs over a time-scale of many orbits, far longer than the dynamical time-scale of the individual black holes. Explicit evolutions of a binary syst…

gr-qc2008★ 195 cited

Binary-black-hole initial data with nearly-extremal spins

Geoffrey Lovelace, Robert Owen, Harald P. Pfeiffer +1

There is a significant possibility that astrophysical black holes with nearly-extremal spins exist. Numerical simulations of such systems require suitable initial data. In this pap…