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19932026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2014 · gr-qcShow all

7 papers · 2 filters

gr-qc2014★ 55 cited

A directed search for gravitational waves from Scorpius X-1 with initial LIGO

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +891

We present results of a search for continuously-emitted gravitational radiation, directed at the brightest low-mass X-ray binary, Scorpius X-1. Our semi-coherent analysis covers 10…

gr-qc2014★ 3.5k cited

Advanced LIGO

The LIGO Scientific Collaboration

The Advanced LIGO gravitational wave detectors are second generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA. The two instru…

gr-qc2014★ 35 cited

Puncture Initial Data for Black-Hole Binaries with High Spins and High Boosts

Ian Ruchlin, James Healy, Carlos O. Lousto +1

We solve the Hamiltonian and momentum constraints of general relativity for two black holes with nearly extremal spins and relativistic boosts in the puncture formalism. We use a n…

gr-qc2014★ 146 cited

Accurate and efficient waveforms for compact binaries on eccentric orbits

E. A. Huerta, Prayush Kumar, Sean T. McWilliams +2

Compact binaries that emit gravitational waves in the sensitivity band of ground-based detectors can have non-negligible eccentricities just prior to merger, depending on the forma…

gr-qc2014★ 42 cited

Detecting gravitational waves from highly eccentric compact binaries

Kai Sheng Tai, Sean T. McWilliams, Frans Pretorius

In dense stellar regions, highly eccentric binaries of black holes and neutron stars can form through various n-body interactions. Such a binary could emit a significant fraction o…

gr-qc2014★ 1 cited

Decline of the current quadrupole moment during the merger phase of binary black hole coalescence

Fan Zhang

Utilizing the tools of tendex and vortex, we study the highly dynamic plunge and merger phases of several -symmetric binary black hole coalescences. In particular, we observe a…