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20162020
most citedGW190521: A Binary Black Hole Merger with a Total Mass of

1.3k citations · 1.6k across the 5 of their papers we have counts for

collaborators

5 papers

gr-qc20201.3k cited

GW190521: A Binary Black Hole Merger with a Total Mass of

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1253

On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio…

gr-qc201877 cited

Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries

Alessandro Nagar, Francesco Messina, Piero Rettegno +5

Spinning neutron stars acquire a quadrupole moment due to their own rotation. This quadratic-in-spin, self-spin effect depends on the equation of state (EOS) and affects the orbita…

astro-ph.HE20182 cited

A crystal ball for kilonovae

Sarp Akcay, Morgan Fraser, Antonio Martin-Carrillo

The discovery of gravitational waves from merging compact objects has opened up a new window to the Universe. Planned third-generation gravitational-wave detectors such as Einstein…

gr-qc201894 cited

Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger

Sarp Akcay, Sebastiano Bernuzzi, Francesco Messina +3

Gravitational-wave astronomy with coalescing binary neutron star sources requires the availability of gravitational waveforms with tidal effects accurate up to merger. This article…

gr-qc201640 cited

Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio

Sarp Akcay, David Dempsey, Sam Dolan

We consider spin-orbit ("geodetic") precession for a compact binary in strong-field gravity. Specifically, we compute , the ratio of the accumulated spin-precession and orbital…