The Third RIT binary black hole simulations catalog

Abstract

The third release of the RIT public catalog of numerical relativity black-hole-binary waveforms \url{http://ccrg.rit.edu/~RITCatalog} consists of 777 accurate simulations that include 300 precessing and 477 nonprecessing binary systems with mass ratios $q=m_1/m_2$ in the range $1/15\le q\le 1$ and individual spins up to $s/m^2=0.95$. The catalog also provides initial parameters of the binary, trajectory information, peak radiation, and final remnant black hole properties. The waveforms are corrected for the center of mass drifting and are extrapolated to future null infinity. We successfully test this correction comparing with simulations of low radition content initial data. As an initial application of this waveform catalog we reanalyze all the peak radiation and remnant properties to find new, simple, correlations among them for practical astrophysical usage.

34 pages, 10 figures, 5 tables

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• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
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• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Study of the Intermediate Mass Ratio Black Hole Binary Merger up to 1000:1 with Numerical Relativity
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Adapted gauge to small mass ratio binary black hole evolutions
• Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sources
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Defining eccentricity for spin-precessing binaries
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Application of the third RIT binary black hole simulations catalog to parameter estimation of gravitational waves signals from the LIGO-Virgo O1/O2 observational runs
• Fundamental Tone and Overtones of Quasinormal Modes in Ringdown Gravitational Waves: A Detailed Study in Black Hole Perturbation
• Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Simulating binary black hole mergers using discontinuous Galerkin methods
• Real modes and null memory contributions in effective-one-body models
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Interplay between numerical relativity and perturbation theory : finite size effects
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Interplay between numerical-relativity and black hole perturbation theory in the intermediate-mass-ratio regime
• Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
• Inferring Binary Properties from Gravitational Wave Signals
• Length dependence of waveform mismatch: a caveat on waveform accuracy
• On the approximate relation between black-hole perturbation theory and numerical relativity
• Numerical evolution of the center of mass and angular momentum for binaries black holes
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications
• A comprehensive look into the accuracy of SpEC binary black hole waveforms
• Final velocity and radiated energy in numerical simulations of binary black holes
• DataVault: A Data Storage Infrastructure for the Einstein Toolkit
• Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries
• AthenaK simulations of the binary black hole merger GW150914
• Comparing numerical relativity and perturbation theory waveforms for a non-spinning equal-mass binary
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits