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20162023
most citedEccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case

129 citations · 596 across the 11 of their papers we have counts for

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19 papers · 1 filter

gr-qc2021

Looking for the parents of LIGO's black holes

Vishal Baibhav, Emanuele Berti, Davide Gerosa +2

Solutions to the two-body problem in general relativity allow us to predict the mass, spin and recoil velocity of a black-hole merger remnant given the masses and spins of its bina…

gr-qc2021

Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics

Christopher J. Moore, Eliot Finch, Riccardo Buscicchio +1

Gravitational-wave observations of binary black holes allow new tests of general relativity to be performed on strong, dynamical gravitational fields. These tests require accurate…

gr-qc2021

A taxonomy of black-hole binary spin precession and nutation

Daria Gangardt, Nathan Steinle, Michael Kesden +2

Binary black holes with misaligned spins will generically induce both precession and nutation of the orbital angular momentum about the total angular momentum . Th…

gr-qc2021129 cited

Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case

Tousif Islam, Vijay Varma, Jackie Lodman +6

We develop new strategies to build numerical relativity surrogate models for eccentric binary black hole systems, which are expected to play an increasingly important role in curre…

gr-qc202014 cited

Up-down instability of binary black holes in numerical relativity

Vijay Varma, Matthew Mould, Davide Gerosa +3

Binary black holes with spins that are aligned with the orbital angular momentum do not precess. However, post-Newtonian calculations predict that "up-down" binaries, in which the…

gr-qc202069 cited

A generalized precession parameter to interpret gravitational-wave data

Davide Gerosa, Matthew Mould, Daria Gangardt +3

Originally designed for waveform approximants, the effective precession parameter is the most commonly used quantity to characterize spin-precession effects in gravi…