A simple model of complete precessing black-hole-binary gravitational waveforms

Abstract

The construction of a model of the gravitational-wave (GW) signal from generic configurations of spinning-black-hole binaries, through inspiral, merger and ringdown, is one of the most pressing theoretical problems in the build-up to the era of GW astronomy. We present the first such model in the frequency domain, "PhenomP", which captures the basic phenomenology of the seven-dimensional parameter space of binary configurations with only three key physical parameters. Two of these (the binary's mass ratio and an effective total spin parallel to the orbital angular momentum, which determines the inspiral rate) define an underlying non-precessing-binary model. The non-precessing-binary waveforms are then "twisted up" with approximate expressions for the precessional motion, which require only one additional physical parameter, an effective precession spin, ${\chi }_p$. All other parameters (total mass, sky location, orientation and polarisation, and initial phase) can be specified trivially. The model is constructed in the frequency domain, which will be essential for efficient GW searches and source measurements. We have tested the model's fidelity for GW applications by comparison against hybrid post-Newtonian-numerical-relativity waveforms at a variety of configurations --although we did not use these numerical simulations in the construction of the model. Our model can be used to develop GW searches, to study the implications for astrophysical measurements, and as a simple conceptual framework to form the basis of generic-binary waveform modelling in the advanced-detector era.

5 pages, 2 figures. Matches version published in PRL

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Cited by in corpus (555)

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• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Rapid and accurate parameter inference for coalescing, precessing compact binaries
• Exploring gravitational-wave detection and parameter inference using Deep Learning methods
• Bayesian model comparison for simulation-based inference
• Astrophysical Prior Information and Gravitational-wave Parameter Estimation
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• High-accuracy simulations of highly spinning binary neutron star systems
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Detection and characterization of spin-orbit resonances in the advanced gravitational wave detectors era
• The reliability of the low-latency estimation of binary neutron star chirp mass
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
• Generic initial data for binary boson stars
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• An architecture for efficient gravitational wave parameter estimation with multimodal linear surrogate models
• Predicting the properties of black holes merger remnants with Deep Neural Networks
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Constrains on the electric charges of the binary black holes with GWTC-1 events
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries
• McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Investigating the noise residuals around the gravitational wave event GW150914
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sources
• Dynamically Formed Black Hole Binaries: In-Cluster Versus Ejected Mergers
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Signs of Higher Multipoles and Orbital Precession in GW151226
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Defining eccentricity for spin-precessing binaries
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Incorporation of model accuracy in gravitational wave Bayesian inference
• SiGMa-Net: Deep learning network to distinguish binary black hole signals from short-duration noise transients
• Deep Learning-based Search for Microlensing Signature from Binary Black Hole Events in GWTC-1 and -2
• Gravitational Wave Beacons
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• 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
• A waveform model for the missing quadrupole mode from black hole coalescence: memory effect and ringdown of the $(\ell =2,m=0)$ spherical harmonic
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Linear vs. nonlinear modeling of black hole ringdowns
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• Universal phenomenological relations between spherical harmonic modes in non-precessing eccentric binary black hole merger waveforms
• Probing resonant excitations in exotic compact objects via gravitational waves
• Characterization of low-significance gravitational-wave compact binary sources
• SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data
• Adaptive mesh refinement in binary black holes simulations
• Inconsistent black hole kick estimates from gravitational-wave models
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• Microlensing bias on the detection of strong lensing gravitational wave
• Improving performance of SEOBNRv3 by $\sim$300x
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Rapid gravitational wave parameter estimation with a single spin: Systematic uncertainties in parameter estimation with the SpinTaylorF2 approximation
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• Numerical Relativity and High Energy Physics: Recent Developments
• Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
• Posterior samples of the parameters of binary black holes from Advanced LIGO, Virgo's second observing run
• Analysis of the subsolar-mass black hole candidate SSM200308 from the second part of the third observing run of Advanced LIGO-Virgo
• Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
• Parameter estimation using a complete signal and inspiral templates for low mass binary black holes with Advanced LIGO sensitivity
• Impact of anti-symmetric contributions to signal multipoles in the measurement of black-hole spins
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• An optimal ${\chi }^2$ discriminator against modelled noise-transients in interferometric data in searches for binary black-hole mergers
• High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
• Gravitational waveforms for high spin and high mass-ratio binary black holes: A synergistic use of numerical-relativity codes
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• An interference-based method for the detection of strongly lensed gravitational waves
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• A Note on QR-Based Model Reduction: Algorithm, Software, and Gravitational Wave Applications
• Gravitational wave extraction in higher dimensional numerical relativity using the Weyl tensor
• Inferring the Astrophysical Population of Gravitational Wave Sources in the Presence of Noise Transients
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Multidimensional hierarchical tests of general relativity with gravitational waves
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Hybrid waveforms for generic precessing binaries for gravitational-wave data analysis
• Mass and tidal parameter extraction from gravitational waves of binary neutron stars mergers using deep learning
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Template-space metric for searches for gravitational waves from the inspiral, merger and ringdown of binary black holes
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Tests of weak equivalence principle with the gravitational wave signals in the LIGO-Virgo catalogue GWTC-1
• Initial Data and Eccentricity Reduction Toolkit for Binary Black Hole Numerical Relativity Waveforms
• Enhancing gravitational waveform models through dynamic calibration
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
• Precessing Binary Black Holes as Better Dark Sirens
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Reducing the number of templates for aligned-spin compact binary coalescence gravitational wave searches using metric-agnostic template nudging
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
• Inferring small neutron star spins with neutron star-black hole mergers
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Testing gravitational waveform models using angular momentum
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Novel Deep Learning Approach to Detecting Binary Black Hole Mergers
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Recent LIGO-Virgo discoveries
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Approaching the black hole by numerical simulations
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• Testing the validity of the phenomenological gravitational waveform models for nonspinning binary black hole searches at low masses
• Accuracy in Measuring the Neutron Star Mass in Gravitational Wave Parameter Estimation for Black Hole-Neutron Star Binaries
• Optimized localization for gravitational-waves from merging binaries
• Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Systematic Bias Due to Nonspinning Template Waveforms in the Gravitational Wave Parameter Estimation for Aligned-Spin Binary Black Holes
• Trumpet Initial Data for Boosted Black Holes
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Inferring the spins of merging black holes in the presence of data-quality issues
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• A full waveform model for arbitrarily axis-symmetric black hole mergers
• Improved binary black hole searches through better discrimination against noise transients
• Gravitational waveform model based on photon motion for spinning black holes
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Constants of motion in gravitational self-force theory
• Optimal follow-up observations of gravitational wave events with small optical telescopes
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Testing black hole metrics with binary black hole inspirals
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Gravitational-wave bursts from spin-precessing black holes in binary systems
• Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
• Pearson cross-correlation in the first four black hole binary mergers
• Tidal deformations of compact objects and gravitational wave emission
• Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution
• Inferences about the distribution, merger rate, and evolutionary processes of compact binaries from gravitational wave observations
• SageNet: Fast Neural Network Emulation of the Stiff-amplified Gravitational Waves from Inflation
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Constraining the Luminosity Function and Delay-Time Distribution of Short Gamma-Ray Bursts for Multimessenger Gravitational-Wave Detection Rate Estimation
• Learning to detect continuous gravitational waves: an open data-analysis competition
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
• Group equivariant neural posterior estimation
• Bounding dark charges on binary black holes using gravitational waves
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
• EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations
• Comparing eccentric waveform models based on post-Newtonian and effective-one-body approaches, over an observationally relevant parameter space
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
• AthenaK simulations of the binary black hole merger GW150914
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• Applying higher-modes consistency test on GW190814 : lessons on no-hair theorem, nature of the secondary compact object and waveform modeling
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Learning Post-Newtonian Corrections from Numerical Relativity
• Parity Violation in Spin-Precessing Binaries: Gravitational Waves from the Inspiral of Black Holes in Dynamical Chern-Simons Gravity
• Extracting the orbital axis from gravitational waves of precessing binary systems
• Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters III: limits from stellar-mass black holes using gravitational-wave observations
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference