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
arXiv:2001.11412 · doi:10.1103/PhysRevD.102.064001
Abstract
In this paper we present IMRPhenomXAS, a thorough overhaul of the IMRPhenomD [1,2] waveform model, which describes the dominant spherical harmonic mode of non-precessing coalescing black holes in terms of piecewise closed form expressions in the frequency domain. Improvements include in particular the accurate treatment of unequal spin effects, and the inclusion of extreme mass ratio waveforms. IMRPhenomD has previously been extended to approximately include spin precession [3] and subdominant spherical harmonics [4], and with its extensions it has become a standard tool in gravitational wave parameter estimation. Improved extensions of IMRPhenomXAS are discussed in companion papers [5,6].
29 pages. 20 figures. Comments and feedback welcome! This paper corresponds to LIGO DCC P2000018
References in corpus (29)
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Advanced LIGO
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
- An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
- Calibration of Moving Puncture Simulations
- Phenomenological template family for black-hole coalescence waveforms
- IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
- Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries
- Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
- Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
- Binary-black-hole initial data with nearly-extremal spins
- High-spin binary black hole mergers
- A multipolar effective one body waveform model for spin-aligned black hole binaries
- Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing
- Binary black hole merger in the extreme mass ratio limit
- Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order
- Cubic order spin effects in the dynamics and gravitational wave energy flux of compact object binaries
- Dynamical Excision Boundaries in Spectral Evolutions of Binary Black Hole Spacetimes
- A new gravitational wave generation algorithm for particle perturbations of the Kerr spacetime
- Binary black hole coalescence in the extreme-mass-ratio limit: testing and improving the effective-one-body multipolar waveform
- Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries
- Dimensional regularization of the IR divergences in the Fokker action of point-particle binaries at the fourth post-Newtonian order
- Gravitational-wave tail effects to quartic non-linear order
- 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
- New frontiers in Numerical Relativity
Cited by in corpus (201)
- 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
- Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
- IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
- New Horizons for Fundamental Physics with LISA
- Real-time gravitational-wave science with neural posterior estimation
- Observation of Gravitational Waves from the Coalescence of a Compact Object and a Neutron Star
- GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
- Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
- Gravitational waveforms for compact binaries from second-order self-force theory
- Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
- Tests of General Relativity with GWTC-3
- GW231123: a Binary Black Hole Merger with Total Mass 190-265
- New twists in compact binary waveform modelling: a fast time domain model for precession
- General-relativistic precession in a black-hole binary
- The Science of the Einstein Telescope
- Effective-one-body waveforms for precessing coalescing compact binaries with post-newtonian Twist
- The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
- IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
- Constraints on Einstein-dilaton-Gauss-Bonnet gravity from Black Hole-Neutron Star Gravitational Wave Events
- Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
- Gravitational-Wave Phasing of Quasi-Circular Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order
- PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
- Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
- A detailed analysis of GW190521 with phenomenological waveform models
- Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
- Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
- A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
- Gravitational waves at the first post-Newtonian order with the Weyssenhoff fluid in Einstein-Cartan theory
- Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
- : a Fisher information matrix Python code for third-generation gravitational-wave detectors
- Gravitational spin-orbit coupling through third-subleading post-Newtonian order: from first-order self-force to arbitrary mass ratios
- Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
- Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation
- GPU-accelerated massive black hole binary parameter estimation with LISA
- The Memory Remains (Undetected): Updates from the Second LIGO/Virgo Gravitational-Wave Transient Catalog
- New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
- Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Possible Causes of False General Relativity Violations in Gravitational Wave Observations
- Follow-up Analyses to the O3 LIGO-Virgo-KAGRA Lensing Searches
- Mode-by-mode Relative Binning: Fast Likelihood Estimation for Gravitational Waveforms with Spin-Orbit Precession and Multiple Harmonics
- The SXS Collaboration's third catalog of binary black hole simulations
- Modelling the Ringdown from Precessing Black Hole Binaries
- Measuring precession in asymmetric compact binaries
- Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
- Validity of common modelling approximations for precessing binary black holes with higher-order modes
- Measuring the spins of heavy binary black holes
- Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
- Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
- Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
- Assessing the model waveform accuracy of gravitational waves
- Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
- Measuring the properties of active galactic nuclei disks with gravitational waves
- High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model
- Revisiting the evidence for precession in GW200129 with machine learning noise mitigation
- VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
- First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
- Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
- Inferring the gravitational wave memory for binary coalescence events
- Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
- Testing gravitational wave propagation with multiband detections
- ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
- Detecting the gravitational wave memory effect with TianQin
- Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
- A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
- Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
- Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
- Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
- Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
- Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
- Efficient multi-timescale dynamics of precessing black-hole binaries
- Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
- Accurate and Efficient Waveform Model for Precessing Binary Black Holes
- Glitch systematics on the observation of massive black-hole binaries with LISA
- Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
- Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
- 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
- Orbital eccentricity in a neutron star - black hole merger
- Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
- Applications of machine learning in gravitational wave research with current interferometric detectors
- High-accuracy waveforms for black hole-neutron star systems with spinning black holes
- On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
- Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
- Post-Newtonian templates for gravitational waves from compact binary inspirals
- Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
- Investigating the effect of in-plane spin directions for Precessing BBH systems
- Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
- Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
- Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
- Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
- Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
- Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
- Space-borne atom interferometric gravitational wave detections. Part III. Eccentricity on dark sirens
- New gravitational waveform model for precessing binary neutron stars with double-spin effects
- Gravitational wave constraints on non-birefringent dispersions of gravitational waves due to Lorentz violations with GWTC-3
- Probabilistic Model for the Gravitational Wave Signal from Merging Black Holes
- Search for eccentric NSBH and BNS mergers in the third observing run of Advanced LIGO and Virgo
- Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
- Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
- Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
- Incorporation of model accuracy in gravitational wave Bayesian inference
- Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
- A waveform model for the missing quadrupole mode from black hole coalescence: memory effect and ringdown of the spherical harmonic
- Constraint on the mass of graviton with gravitational waves
- Assessing gravitational-wave binary black hole candidates with Bayesian odds
- Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
- Observational limits on the rate of radiation-driven binary black hole capture events
- Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling
- Strong Field Scattering of Black Holes: Assessing Resummation Strategies
- Inconsistent black hole kick estimates from gravitational-wave models
- Revealing the - Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers
- Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
- Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
- Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge
- Testing alternative theories of gravity with space-based gravitational wave detectors
- Source localizations with the network of space-based gravitational wave detectors
- Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
- Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
- Computational Techniques for Parameter Estimation of Gravitational Wave Signals
- GPU-accelerated LISA parameter estimation with full time domain response
- Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
- Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
- High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
- Multidimensional hierarchical tests of general relativity with gravitational waves
- Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
- Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
- Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
- Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
- Symplectic mechanics of relativistic spinning compact bodies II.: Canonical formalism in the Schwarzschild spacetime
- Extending superposed harmonic initial data to higher spin
- Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
- Forecasting the population properties of merging black holes
- Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
- Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
- Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
- Inferring small neutron star spins with neutron star-black hole mergers
- Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
- Observability of spin precession in the presence of a black-hole remnant kick
- Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
- Testing gravitational waveform models using angular momentum
- Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
- Success of the small mass ratio approximation during the final orbits of binary black hole simulations
- Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
- Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
- Fast and faithful interpolation of numerical relativity surrogate waveforms using meshfree approximation
- Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
- Recent LIGO-Virgo discoveries
- Vetting quark-star models with gravitational waves in the hierarchical Bayesian framework
- Gravitational waves from quasielliptic compact binaries in scalar-tensor theory to one-and-a-half post-Newtonian order
- The directional isotropy of LIGO-Virgo binaries
- Advancing the Effective-One-Body Framework in the Test-Mass Limit
- Black-Hole Perturbation Plus Post-Newtonian Theory: Hybrid Waveform for Neutron Star Binaries
- Spectrogram correlated stacking: A novel time-frequency domain analysis of the Stochastic Gravitational Wave Background
- Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
- Systematic biases in parameter estimation on LISA binaries: The effect of excluding higher harmonics for non-spinning binaries
- Testing modified gravity with the eccentric neutron star--black hole merger GW200105
- Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
- Probing Spin-Orbit Resonances with the Binary Black Hole Population
- Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
- Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
- Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
- Projected gravitational wave constraints on primordial black hole abundance for extended mass distributions
- Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
- Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
- Unmasking noise transients masquerading as intermediate-mass black hole binaries
- Tests of general relativity at the fourth post-Newtonian order
- Calibrating approximate Bayesian credible intervals of gravitational-wave parameters
- Asymptotically matched quasi-circular inspiral and transition-to-plunge in the small mass ratio expansion
- Primordial black holes with mass ratio-modulated initial clustering: merger suppression and projected constraints
- A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
- A Parametrized Test of General Relativity for LISA Massive Black Hole Binary Inspirals
- Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
- Primordial black holes versus their impersonators at gravitational wave observatories
- Challenging a binary neutron star merger interpretation of GW230529
- The impact of precession and higher-order multipoles for gravitational wave cosmological inference
- Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
- Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
- Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
- Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries
- Secular evolution of orbital parameters for general bound orbits in Kerr spacetime
- Glitch veto based on unphysical gravitational wave binary inspiral templates
- The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
- Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
- Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
- Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
- Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge
- Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
- Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
- AthenaK simulations of the binary black hole merger GW150914
- Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
- Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
- Applying higher-modes consistency test on GW190814 : lessons on no-hair theorem, nature of the secondary compact object and waveform modeling
- Learning Post-Newtonian Corrections from Numerical Relativity
- Could the high-mass black holes from gravitational-wave observations be explained by lensing?
- labrador: A domain-optimized machine-learning tool for gravitational wave inference
- Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
- Characterization of merging black holes with two precessing spins
- Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
- Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling