Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
arXiv:2502.17400 · doi:10.1103/nkq9-zh2y
Abstract
The PE for GW merger events relies on a waveform model calibrated using numerical simulations. Within the Bayesian framework, this waveform model represents the GW signal produced during the merger and is crucial for estimating the likelihood function. However, these waveform models may possess systematic errors that can differ across the parameter space. Addressing these errors in the current data analysis pipeline is an active area of research. We introduce parametrizations for the uncertainties in the amplitude and phase of the reference waveform model. When the error budget in the amplitude and phase of the waveform model, as a function of frequency, is known, it can be used as a prior distribution in the Bayesian framework. We also show that conservative priors can be used to quantify uncertainties in waveform modeling without any knowledge of waveform uncertainty error budgets. Through zero-noise injections and PE recoveries, we demonstrate that even 1%-2% of errors in relative phase to the actual waveform model, for a GW150914-like signal and advanced LIGO detector sensitivity, can introduce biases in the recovered parameters. These biases can be corrected when we account for waveform uncertainties within the PE framework. By analyzing a series of simulated signals from mergers with precessing orbits and recovering them using a non-spinning waveform model, we demonstrate that we can reduce the ratio of systematic errors to statistical errors. This approach allows us to address scenarios where specific physical effects are missing in waveform modeling. The code that implements our parametrization for performing PE is available as a Python package "pycbc_wferrors_plugin", compatible with the PyCBC open source GW analysis library.
24 pages, 13 figures, 3 tables. Matches with the accepted version of the manuscript
References in corpus (97)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- 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
- GW170817: Measurements of Neutron Star Radii and Equation of State
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- Evolution of Binary Black Hole Spacetimes
- Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
- Effective one-body approach to general relativistic two-body dynamics
- Gravitational wave extraction from an inspiraling configuration of merging black holes
- Properties of the binary neutron star merger GW170817
- Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
- A simple model of complete precessing black-hole-binary gravitational waveforms
- GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
- The PyCBC search for gravitational waves from compact binary coalescence
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
- 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
- Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy
- Effective-one-body model for black-hole binaries with generic mass ratios and spins
- 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
- Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
- Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory
- Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
- A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
- A chi-squared time-frequency discriminator for gravitational wave detection
- Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
- Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
- IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
- Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
- PyCBC Inference: A Python-based parameter estimation toolkit for compact binary coalescence signals
- Surrogate model of hybridized numerical relativity binary black hole waveforms
- Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
- Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
- First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
- Constraints on the cosmic expansion history from GWTC-3
- 4-OGC: Catalog of gravitational waves from compact-binary mergers
- Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
- Fast prediction and evaluation of gravitational waveforms using surrogate models
- A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
- LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
- Including higher order multipoles in gravitational-wave models for precessing binary black holes
- Improved effective-one-body description of coalescing nonspinning black-hole binaries and its numerical-relativity completion
- Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
- A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
- Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
- Characterization of systematic error in Advanced LIGO calibration
- Forecasting the detection capabilities of third-generation gravitational-wave detectors using
- Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
- New twists in compact binary waveform modelling: a fast time domain model for precession
- Science-Driven Tunable Design of Cosmic Explorer Detectors
- IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
- Template-based searches for gravitational waves: efficient lattice covering of flat parameter spaces
- PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
- : a Fisher information matrix Python code for third-generation gravitational-wave detectors
- Waveform systematics for binary neutron star gravitational wave signals: effects of the point-particle baseline and tidal descriptions
- Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
- Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
- Possible Causes of False General Relativity Violations in Gravitational Wave Observations
- Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
- Novel Method for Incorporating Model Uncertainties into Gravitational Wave Parameter Estimates
- Spin effects in gravitational waveforms and fluxes for binaries on eccentric orbits to the third post-Newtonian order
- Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
- Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
- Assessing the model waveform accuracy of gravitational waves
- Multi-waveform inference of gravitational waves
- Analytical meets numerical relativity - status of complete gravitational waveform models for binary black holes
- Waveform systematics for binary neutron star gravitational wave signals: Effects of spin, precession, and the observation of electromagnetic counterparts
- Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
- First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
- ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
- Optimal Template Banks
- Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
- Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
- Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
- The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
- Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1
- Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
- Understanding binary neutron star collisions with hypermodels
- Probabilistic Model for the Gravitational Wave Signal from Merging Black Holes
- Incorporation of model accuracy in gravitational wave Bayesian inference
- Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
- Validating Prior-informed Fisher-matrix Analyses against GWTC Data
- Problematic systematics in neutron-star merger simulations
- Parameter Estimation with Nonstationary Noise in Gravitational-wave Data