output
19922025
most citedGWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

3.5k citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 2017 · gr-qcShow all

5 papers · 2 filters

gr-qc2017★ 108 cited

Gravitational-wave luminosity of binary neutron stars mergers

Francesco Zappa, Sebastiano Bernuzzi, David Radice +2

We study the gravitational-wave peak luminosity and radiated energy of quasicircular neutron star mergers using a large sample of numerical relativity simulations with different bi…

gr-qc2017★ 42 cited

Numerical Relativity Simulations of Precessing Binary Neutron Star Mergers

Tim Dietrich, Sebastiano Bernuzzi, Bernd Bruegmann +2

We present the first set of numerical relativity simulations of binary neutron mergers that include spin precession effects and are evolved with multiple resolutions. Our simulatio…

gr-qc2017★ 239 cited

GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1099

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron…

gr-qc2017★ 44 cited

Spectral analysis of gravitational waves from binary neutron star merger remnants

Francesco Maione, Roberto De Pietri, Alessandra Feo +1

In this work we analyze the gravitational wave signal from hypermassive neutron stars formed after the merger of binary neutron star systems, focusing on its spectral features. The…

gr-qc2017★ 251 cited

Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations

Tim Dietrich, Sebastiano Bernuzzi, Wolfgang Tichy

We construct closed-form gravitational waveforms (GWs) with tidal effects for the coalescence and merger of binary neutron stars. The method relies on a new set of eccentricity-red…