most citedToward faithful templates for non-spinning binary black holes using the effective-one-body approach

286 citations · 933 across the 6 of their papers we have counts for

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gr-qc2007144 cited

Anatomy of the binary black hole recoil: A multipolar analysis

Jeremy D. Schnittman, Alessandra Buonanno, James R. van Meter +5

We present a multipolar analysis of the gravitational recoil computed in recent numerical simulations of binary black hole (BH) coalescence, for both unequal masses and non-zero, n…

gr-qc2007286 cited

Toward faithful templates for non-spinning binary black holes using the effective-one-body approach

Alessandra Buonanno, Yi Pan, John G. Baker +4

We present an accurate approximation of the full gravitational radiation waveforms generated in the merger of non-eccentric systems of two non-spinning black holes. Utilizing infor…

gr-qc2007176 cited

A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case

Yi Pan, Alessandra Buonanno, John G. Baker +5

We compare waveforms obtained by numerically evolving nonspinning binary black holes to post-Newtonian (PN) template families currently used in the search for gravitational waves b…

gr-qc2007195 cited

Upper limits on gravitational wave emission from 78 radio pulsars

The LIGO Scientific Collaboration, B. Abbott, M. Kramer +1

We present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO600 gravitational wave dete…

gr-qc200699 cited

Binary black hole late inspiral: Simulations for gravitational wave observations

John G. Baker, Sean T. McWilliams, James R. van Meter +4

Coalescing binary black hole mergers are expected to be the strongest gravitational wave sources for ground-based interferometers, such as the LIGO, VIRGO, and GEO600, as well as t…

gr-qc2006159 cited

Consistency of post-Newtonian waveforms with numerical relativity

John G. Baker, James R. van Meter, Sean T. McWilliams +2

General relativity predicts the gravitational wave signatures of coalescing binary black holes. Explicit waveform predictions for such systems, required for optimal analysis of obs…