Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model

Abstract

The plunge-merger stage of the binary-black hole coalescence, when the bodies' velocities reach a large fraction of the speed of light and the gravitational-wave luminosity peaks, provides a unique opportunity to probe gravity in the dynamical and nonlinear regime. How much do the predictions of general relativity differ from the ones in other theories of gravity for this stage of the binary evolution? To address this question, we develop a parametrized waveform model, within the effective-one-body formalism, that allows for deviations from general relativity in the plunge-merger-ringdown stage. As first step, we focus on nonprecessing-spin, quasicircular black hole binaries. In comparison to previous works, for each gravitational wave mode, our model can modify, with respect to general-relativistic predictions, the instant at which the amplitude peaks, the instantaneous frequency at this time instant, and the value of the peak amplitude. We use this waveform model to explore several questions considering both synthetic-data injections and two gravitational wave signals. In particular, we find that deviations from the peak gravitational wave amplitude and instantaneous frequency can be constrained to about $20\%$ with GW150914. Alarmingly, we find that GW200129_065458 shows a strong violation of general relativity. We interpret this result as a false violation, either due to waveform systematics (mismodeling of spin precession) or due to data-quality issues depending on one's interpretation of this event. This illustrates the use of parametrized waveform models as tools to investigate systematic errors in plain general relativity. The results with GW200129_065458 also vividly demonstrate the importance of waveform systematics and of glitch mitigation procedures when interpreting tests of general relativity with current gravitational wave observations.

arXiv comment17+4 pages, 16 figures. v3: matches published version

References in corpus (115)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Modified Gravity and Cosmology
• The Confrontation between General Relativity and Experiment
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• Advanced LIGO
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• Tests of general relativity with GW150914
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
• Effective one-body approach to general relativistic two-body dynamics
• Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
• Properties of the Binary Black Hole Merger GW150914
• Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• Transition from inspiral to plunge in binary black hole coalescences
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
• Observation of gravitational waves from two neutron star-black hole coalescences
• First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• Tests of General Relativity with GW170817
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
• Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
• Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework
• On the determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• The SXS Collaboration catalog of binary black hole simulations
• A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
• Surrogate models for precessing binary black hole simulations with unequal masses
• Testing the no-hair theorem with GW150914
• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
• Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
• Transition from inspiral to plunge in precessing binaries of spinning black holes
• Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries
• Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
• Strong-field Gravity Tests with the Double Pulsar
• Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• Gravitational Wave Tests of General Relativity with the Parameterized Post-Einsteinian Framework
• New Test of the Gravitational $1/r^2$ Law at Separations down to 52 $\mu$m
• Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries
• Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-spinning, equal-mass black holes
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries
• Observational Black Hole Spectroscopy: A time-domain multimode analysis of GW150914
• Bayesian model selection for testing the no-hair theorem with black hole ringdowns
• Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics
• A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case
• Improved effective-one-body description of coalescing nonspinning black-hole binaries and its numerical-relativity completion
• Testing post-Newtonian theory with gravitational wave observations
• Probing the non-linear structure of general relativity with black hole binaries
• High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
• Testing general relativity using golden black-hole binaries
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Testing the no-hair theorem with black hole ringdowns using TIGER
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
• Dynamics of spontaneous black hole scalarization and mergers in Einstein-scalar-Gauss-Bonnet gravity
• Numerical binary black hole mergers in dynamical Chern-Simons: I. Scalar field
• Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of binary black holes
• A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
• Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation
• Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity
• Parameter estimation of spinning binary inspirals using Markov-chain Monte Carlo
• General-relativistic precession in a black-hole binary
• Constraints on quasi-normal-mode frequencies with LIGO-Virgo binary-black-hole observations
• Dynamical descalarization in binary black hole mergers
• Numerical relativity simulation of GW150914 beyond general relativity
• Numerical binary black hole collisions in dynamical Chern-Simons gravity
• Empirical tests of the black hole no-hair conjecture using gravitational-wave observations
• Effective-one-body waveforms for precessing coalescing compact binaries with post-newtonian Twist
• The curious case of GW200129: interplay between spin-precession inference and data-quality issues
• Modeling multipolar gravitational-wave emission from small mass-ratio mergers
• Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Small mass plunging into a Kerr black hole: Anatomy of the inspiral-merger-ringdown waveforms
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• Hierarchical test of general relativity with gravitational waves
• Black-hole ringdown as a probe of higher-curvature gravity theories
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Nonlinear studies of binary black hole mergers in Einstein-scalar-Gauss-Bonnet gravity
• Golden Binary Gravitational-Wave Sources: Robust Probes of Strong-Field Gravity
• Accelerating parameter inference with graphics processing units
• Constraining gravitational wave amplitude birefringence and Chern-Simons gravity with GWTC-2
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Systematic bias on parameterized tests of general relativity due to neglect of orbital eccentricity
• Spin-induced dynamical scalarization, de-scalarization and stealthness in scalar-Gauss-Bonnet gravity during black hole coalescence
• Bayesian inference on compact binary inspiral gravitational radiation signals in interferometric data
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• Well-posedness of the four-derivative scalar-tensor theory of gravity in singularity avoiding coordinates
• Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
• Systematic bias on the inspiral-merger-ringdown consistency test due to neglect of orbital eccentricity
• Stealth Bias in Gravitational-Wave Parameter Estimation
• Comparing Effective One Body Hamiltonians for spin-aligned coalescing binaries
• Black Hole Binaries in Cubic Horndeski Theories
• Parametrized tests of post-Newtonian theory using principal component analysis
• Dynamical descalarization with a jump during black hole merger
• Search for anisotropic, birefringent spacetime-symmetry breaking in gravitational wave propagation from GWTC-3
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• Investigating the relation between gravitational wave tests of general relativity
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Gravitational wave inference on a numerical-relativity simulation of a black hole merger beyond general relativity
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Merger-Ringdown Consistency: A New Test of Strong Gravity using Deep Learning
• GW150914 peak frequency: a novel consistency test of strong-field General Relativity
• Arrival Times of Gravitational Radiation Peaks for Binary Inspiral

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• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
• The Science of the Einstein Telescope
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• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
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• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Linear vs. nonlinear modeling of black hole ringdowns
• GRFolres: A code for modified gravity simulations in strong gravity
• Quasinormal modes of slowly-spinning horizonless compact objects
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Catalog variance of testing general relativity with gravitational-wave data
• Theory-agnostic searches for non-gravitational modes in black hole ringdown
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• Quasi-normal modes of slowly-rotating Johannsen black holes
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• A Parametrized Test of General Relativity for LISA Massive Black Hole Binary Inspirals
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• Neutron stars as extreme gravity probes
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Probing missing physics from inspiralling compact binaries via time-frequency tracks