Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM

Abstract

Gravitational waves from compact binary coalescence sources can be decomposed into spherical-harmonic multipoles, the dominant being the quadrupole ($\ell =2,m=\pm 2$) modes. The contribution of sub-dominant modes towards total signal power increases with increasing binary mass ratio and source inclination to the detector. It is well-known that in these cases neglecting higher modes could lead to measurement biases, but these have not yet been quantified with a higher-mode model that includes spin effects. In this study, we use the multi-mode aligned-spin phenomenological waveform model IMRPhenomHM to investigate the effects of including multi-mode content in estimating source parameters and contrast the results with using a quadrupole-only model (IMRPhenomD). We use as sources IMRPhenomHM and hybrid EOB-NR waveforms over a range of mass-ratio and inclination combinations, and recover the parameters with IMRPhenomHM and IMRPhenomD. These allow us to quantify the accuracy of parameter measurements using a multi-mode model, the biases incurred when using a quadrupole-only model to recover full (multi-mode) signals, and the systematic errors in the IMRPhenomHM model. We see that the parameters recovered by multi-mode templates are more precise for all non-zero inclinations as compared to quadrupole templates. For multi-mode injections, IMRPhenomD recovers biased parameters for non-zero inclinations with lower likelihood while IMRPhenomHM recovered parameters are accurate for most cases, and if a bias exists, it can be explained as a combined effect of observational priors and (in the case of hybrid-NR signals) waveform inaccuracies. For cases where IMRPhenomHM recovers biased parameters, the bias is always smaller than the corresponding IMRPhenomD recovery, and we conclude that IMRPhenomHM will be sufficiently accurate to allow unbiased measurements for most GW observations.

arXiv comment14 pages, 7 figures

References in corpus (59)

• 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
• 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
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Characterization of the LIGO detectors during their sixth science run
• 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
• 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
• Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
• The SXS Collaboration catalog of binary black hole simulations
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• Surrogate models for precessing binary black hole simulations with unequal masses
• Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
• Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
• The LIGO Open Science Center
• Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
• BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
• 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
• Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and non-precessing inspiral signals
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models
• A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
• Degeneracy between mass and spin in black-hole-binary waveforms
• Tracking the precession of compact binaries from their gravitational-wave signal
• Source localization with an advanced gravitational wave detector network
• A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
• Effects of waveform model systematics on the interpretation of GW150914
• A geometric approach to the precession of compact binaries
• A tapering window for time-domain templates and simulated signals in the detection of gravitational waves from coalescing compact binaries
• Gravitational-wave observations of binary black holes: Effect of non-quadrupole modes
• On the properties of the massive binary black hole merger GW170729
• Impact of Higher Harmonics in Searching for Gravitational Waves from Non-Spinning Binary Black Holes
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries
• Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes
• Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation
• Binary black hole spectroscopy
• Detectability of gravitational waves from binary black holes: Impact of precession and higher modes
• Searching for the full symphony of black hole binary mergers
• Energetics and phasing of nonprecessing spinning coalescing black hole binaries
• Effects of nonquadrupole modes in the detection and parameter estimation of black hole binaries with nonprecessing spins
• Systematic biases in parameter estimation of binary black-hole mergers
• Constraining black-hole spins with gravitational wave observations
• Parameter Estimation of Gravitational Waves from Precessing BH-NS Inspirals with higher harmonics
• Nonspinning searches for spinning binaries in ground-based detector data: Amplitude and mismatch predictions in the constant precession cone approximation
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• Parameter Estimation of Gravitational Waves from Nonprecessing BH-NS Inspirals with higher harmonics: Comparing MCMC posteriors to an Effective Fisher Matrix
• Accurate inspiral-merger-ringdown gravitational waveforms for non-spinning black-hole binaries including the effect of subdominant modes
• Impact of Numerical Relativity information on effective-one-body waveform models
• Numerical Relativity Injection Infrastructure
• Including mode mixing in a higher-multipole model for gravitational waveforms from nonspinning black-hole binaries
• Comparison of subdominant gravitational wave harmonics between post-Newtonian and numerical relativity calculations and construction of multi-mode hybrids

Cited by in corpus (47)

• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Measuring gravitational-wave higher-order modes
• $\text{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors
• Identifying Type II Strongly Lensed Gravitational-Wave Images in Third-Generation Gravitational-Wave Detectors
• GPU-accelerated massive black hole binary parameter estimation with LISA
• Mode-by-mode Relative Binning: Fast Likelihood Estimation for Gravitational Waveforms with Spin-Orbit Precession and Multiple Harmonics
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• The SXS Collaboration's third catalog of binary black hole simulations
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Identifying when Precession can be Measured in Gravitational Waveforms
• Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
• The Importance of Priors on LIGO-Virgo Parameter Estimation: the Case of Primordial Black Holes
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Inconsistent black hole kick estimates from gravitational-wave models
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Detectability of gravitational higher order modes in the third-generation era
• Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
• Black-box density function estimation using recursive partitioning
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission