The RIT binary black hole simulations catalog

Abstract

The RIT numerical relativity group is releasing a public catalog of black-hole-binary waveforms. The initial release of the catalog consists of 126 recent simulations that include precessing and non precessing systems with mass ratios $q=m_1/m_2$ in the range $1/6\le q\le 1$. The catalog contains information about the initial data of the simulation, the waveforms extrapolated to infinity, as well as information about the peak luminosity and final remnant black hole properties. These waveforms can be used to independently interpret gravitational wave signals from laser interferometric detectors and

5 pages, 3 figures

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• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Gravitational Wave Denoising of Binary Black Hole Mergers with Deep Learning
• On the properties of the massive binary black hole merger GW170729
• Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• The second RIT binary black hole simulations catalog and its application to gravitational waves parameter estimation
• Adding Gravitational Memory to Waveform Catalogs using BMS Balance Laws
• Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• The Third RIT binary black hole simulations catalog
• High Precision Ringdown Modeling: Multimode Fits and BMS Frames
• Machine Learning Gravitational Waves from Binary Black Hole Mergers
• Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
• Second release of the CoRe database of binary neutron star merger waveforms
• Fixing the BMS Frame of Numerical Relativity Waveforms
• The SXS Collaboration's third catalog of binary black hole simulations
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• The hangup effect in unequal mass binary black hole mergers and further studies of their gravitational radiation and remnant properties
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Physics of eccentric binary black hole mergers: A numerical relativity perspective
• Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
• Comparison of various methods to extract ringdown frequency from gravitational wave data
• Simple procedures to reduce eccentricity of binary black hole simulations
• Ringdown frequencies in black holes formed from precessing black-hole binaries
• First gravitational-wave search for intermediate-mass black hole mergers with higher order harmonics
• Optimization of model independent gravitational wave search using machine learning
• Numerical relativity in spherical coordinates with the Einstein Toolkit
• Comparing Remnant Properties from Horizon Data and Asymptotic Data in Numerical Relativity
• Targeted numerical simulations of binary black holes for GW170104
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Characterization of numerical relativity waveforms of eccentric binary black hole mergers
• Study of the Intermediate Mass Ratio Black Hole Binary Merger up to 1000:1 with Numerical Relativity
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Rapid and accurate parameter inference for coalescing, precessing compact binaries
• Initial data for general relativistic simulations of multiple electrically charged black holes with linear and angular momenta
• 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
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sources
• Spontaneous creation of circularly polarized photons in chiral astrophysical systems
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing
• BOSS-LDG: A Novel Computational Framework that Brings Together Blue Waters, Open Science Grid, Shifter and the LIGO Data Grid to Accelerate Gravitational Wave Discovery
• Gravitational Wave Beacons
• 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
• Adaptive mesh refinement in binary black holes simulations
• Fundamental Tone and Overtones of Quasinormal Modes in Ringdown Gravitational Waves: A Detailed Study in Black Hole Perturbation
• Evolutions of unequal mass, highly spinning black hole binaries
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Simulating binary black hole mergers using discontinuous Galerkin methods
• Gravitational waveforms for high spin and high mass-ratio binary black holes: A synergistic use of numerical-relativity codes
• Black Hole Spin Axis in Numerical Relativity
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Real modes and null memory contributions in effective-one-body models
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Interplay between numerical relativity and perturbation theory : finite size effects
• Black hole spectroscopy for KAGRA future prospect in O5
• Efficient simulations of high-spin black holes with a new gauge
• Hybrid waveforms for generic precessing binaries for gravitational-wave data analysis
• Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits
• Initial Data and Eccentricity Reduction Toolkit for Binary Black Hole Numerical Relativity Waveforms
• 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
• Length dependence of waveform mismatch: a caveat on waveform accuracy
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Adapted gauge to a quasilocal measure of the black holes recoil
• On the approximate relation between black-hole perturbation theory and numerical relativity
• Approaching the black hole by numerical simulations
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Numerical evolution of the center of mass and angular momentum for binaries black holes
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Rio: A new computational framework for accurate initial data of binary black holes
• 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
• Comparing numerical relativity and perturbation theory waveforms for a non-spinning equal-mass binary
• AthenaK simulations of the binary black hole merger GW150914
• Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits
• The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
• New numerical framework for the generalized Baumgarte-Shapiro-Shibata-Nakamura formulation: The vacuum case for spherical symmetry
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms