Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
arXiv:2203.02670 · doi:10.3847/1538-4357/ac6b99
Abstract
The Fisher information matrix (FM) plays an important role in forecasts and inferences in many areas of physics. While giving fast parameter estimation with the Gaussian likelihood approximation in the parameter space, the FM can only give the ellipsoidal posterior contours of parameters and lose the higher-order information beyond Gaussianity. We extend the FM in gravitational-wave (GW) data analysis using the Derivative Approximation for LIkelihoods (DALI), a method to expand the likelihood while keeping it positive definite and normalizable at every order, for more accurate forecasts and inferences. When applied to the two real GW events, GW150914 and GW170817, DALI can reduce the difference between FM approximation and the real posterior by 5 times in the best case. The calculation time of DALI and FM is at the same order of magnitude, while obtaining the real full posterior will take several orders of magnitude longer. Besides more accurate approximations, higher-order correction from DALI provides a fast assessment on the FM analysis and gives suggestions for complex sampling techniques which are computationally intensive. We recommend using the DALI method as an extension to the FM method in GW data analysis to pursue better accuracy while still keeping the speed.
arXiv comment11 pages, 2 figures; accepted by ApJ
References in corpus (37)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- emcee: The MCMC Hammer
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- 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
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
- 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
- Detection, Measurement and Gravitational Radiation
- Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Angular Resolution of the LISA Gravitational Wave Detector
- Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
- Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
- Estimating spinning binary parameters and testing alternative theories of gravity with LISA
- Real-time gravitational-wave science with neural posterior estimation
- Massively parallel Bayesian inference for transient gravitational-wave astronomy
- Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
- The LISA-Taiji network
- Science with the TianQin observatory: Preliminary results on massive black hole binaries
- Learning Bayesian posteriors with neural networks for gravitational-wave inference
- Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
- Heterodyned Likelihood for Rapid Gravitational Wave Parameter Inference
- Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
- Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
- Beyond Fisher: exact sampling distributions of the maximum-likelihood estimator in gravitational-wave parameter estimation
- Forecasts of non-Gaussian parameter spaces using Box-Cox transformations
- A fast, always positive definite and normalizable approximation of non-Gaussian likelihoods
- Application of asymptotic expansions of maximum likelihood estimators errors to gravitational waves from binary mergers: the single interferometer case
- Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks
- Neutron StarNeutron Star and Neutron StarBlack Hole Mergers: Multiband Observations and Early Warnings
- Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
- Prospects for detecting exoplanets around double white dwarfs with LISA and Taiji
- Non-Gaussian forecasts of weak lensing with and without priors
Cited by in corpus (11)
- The Science of the Einstein Telescope
- : a Fisher information matrix Python code for third-generation gravitational-wave detectors
- Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
- Prospects for Constraining the Yukawa Gravity with Pulsars around Sagittarius A*
- Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
- Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
- Simultaneous bounds on the gravitational dipole radiation and varying gravitational constant from compact binary inspirals
- GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
- Prospects for detecting neutron star-white dwarf mergers with decihertz gravitational-wave observatories
- Beyond Fisher Forecasting for Cosmology
- Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network