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19952019
most citedAccurate Evolutions of Orbiting Black-Hole Binaries Without Excision

1.4k citations · 3.1k across the 20 of their papers we have counts for

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20 papers

astro-ph.HE2019★ 70 cited

Quasi-Periodicity of Supermassive Binary Black Hole Accretion Approaching Merger

Dennis B. Bowen, Vassilios Mewes, Scott C. Noble +3

In this paper we continue the first ever study of magnetized mini-disks coupled to circumbinary accretion in a supermassive binary black hole (SMBBH) approaching merger reported in…

astro-ph.HE2018★ 93 cited

Quasi-Periodic Behavior of Mini-Disks in Binary Black Holes Approaching Merger

Dennis B. Bowen, Vassilios Mewes, Manuela Campanelli +3

We present the first magnetohydrodynamic simulation in which a circumbinary disk around a relativistic binary black hole feeds mass to individual accretion disks ("mini-disks") aro…

gr-qc2017★ 85 cited

A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity

Jacob Lange, Richard O'Shaughnessy, Michael Boyle +23

We present and assess a Bayesian method to interpret gravitational wave signals from binary black holes. Our method directly compares gravitational wave data to numerical relativit…

gr-qc2010★ 7 cited

Perturbative effects of spinning black holes with applications to recoil velocities

Hiroyuki Nakano, Manuela Campanelli, Carlos O. Lousto +1

Recently, we proposed an enhancement of the Regge-Wheeler-Zerilli formalism for first-order perturbations about a Schwarzschild background that includes first-order corrections due…

gr-qc2010★ 29 cited

Modeling Gravitational Recoil Using Numerical Relativity

Yosef Zlochower, Manuela Campanelli, Carlos O. Lousto

We review the developments in modeling gravitational recoil from merging black-hole binaries and introduce a new set of 20 simulations to test our previously proposed empirical for…

gr-qc2009

Comparison of Post-Newtonian and Numerical Evolutions of Black-Hole Binaries

Hiroyuki Nakano, Manuela Campanelli, Carlos O. Lousto +1

In this paper, we compare the waveforms from the post-Newtonian (PN) approach with the numerical simulations of generic black-hole binaries which have mass ratio , arbitr…