Upgraded waveform model of eccentric binary black hole based on effective-one-body-numerical-relativity for spin-aligned binary black holes

Abstract

Effective one body numerical relativity waveform models for spin aligned binary black holes (SEOBNR) are based on the effective one body theoretical framework and numerical relativity simulation results. SEOBNR models have evolved through version 1 to version 4. We recently extended SEOBNRv1 model to SEOBNRE (Effective One Body Numerical Relativity waveform models for Spin aligned binary black holes along Eccentric orbit) model which is also valid for spin aligned binary black hole coalescence along eccentric orbit. In this paper we update our previous SEOBNRE model to make it consistent to SEOBNRv4 which is the most widely used SEOBNR waveform model. This upgraded SEOBNRE model improves accuracy compared to previous SEOBNRE model, especially for highly spinning black holes. For spin aligned binary black holes with mass ratio $1\le q\lesssim 10$, dimensionless spin $-0.9\lesssim \chi \lesssim 0.995$ and orbital eccentricity $0\le e_0\lesssim 0.6$ at reference frequency $M{f}_0=0.002$ ($M$ is the total mass of the binary black hole, $f_0\approx 40\frac{10{\mathrm{M}}_{\odot }}{M}$Hz), the upgraded SEOBNRE model can always fit numerical relativity waveform better than 98.2\%. For most cases the fitting factor can even be better than 99\%.

arXiv comment15 pages, 10 figures

References in corpus (78)

• TianQin: a space-borne gravitational wave detector
• Effective one-body approach to general relativistic two-body dynamics
• The construction and use of LISA sensitivity curves
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• Formation and Evolution of Compact Object Binaries in AGN Disks
• 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
• Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• 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
• A Highly Spinning and Aligned Binary Black Hole Merger in the Advanced LIGO First Observing Run
• 1-OGC: The first open gravitational-wave catalog of binary mergers from analysis of public Advanced LIGO data
• Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation
• A New Search Pipeline for Compact Binary Mergers: Results for Binary Black Holes in the First Observing Run of Advanced LIGO
• The First Round Result from the TianQin-1 Satellite
• A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
• A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
• The LISA-Taiji network
• Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
• Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• Self consistent model for the evolution of eccentric massive black hole binaries in stellar environments: implications for gravitational wave observations
• Searching for Eccentricity: Signatures of Dynamical Formation in the First Gravitational-Wave Transient Catalogue of LIGO and Virgo
• Accurate and efficient waveforms for compact binaries on eccentric orbits
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order
• An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory
• Complete waveform model for compact binaries on eccentric orbits
• Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO
• Comparisons of eccentric binary black hole simulations with post-Newtonian models
• Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits
• Charge-induced force-noise on free-falling test masses: results from LISA Pathfinder
• Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
• Binary black hole merger in the extreme-mass-ratio limit: a multipolar analysis
• Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger
• Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Modeling multipolar gravitational-wave emission from small mass-ratio mergers
• A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
• Radiation-reaction force and multipolar waveforms for eccentric, spin-aligned binaries in the effective-one-body formalism
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Effect of eccentricity on binary neutron star searches in Advanced LIGO
• On the origin of GW190425
• Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries
• Detecting Intermediate-Mass Ratio Inspirals From The Ground And Space
• Search for Eccentric Binary Neutron Star Mergers in the first and second observing runs of Advanced LIGO
• Effective-one-body waveforms for binary neutron stars using surrogate models
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Third post-Newtonian gravitational waveforms for compact binary systems in general orbits: Instantaneous terms
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• Measuring the eccentricity of GW170817 and GW190425
• Parameter estimation for inspiraling eccentric compact binaries including pericenter precession
• Numerical simulation of sky localization for LISA-TAIJI joint observation
• A Parametrized post-Einsteinian Framework for Gravitational Wave Bursts
• Measuring eccentricity of binary black holes in GWTC-1 by using inspiral-only waveform
• Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
• A Rosetta Stone for eccentric gravitational waveform models
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Eccentric Gravitational Wave Bursts in the Post-Newtonian Formalism
• Intermediate-mass-ratio black hole binaries II: Modeling Trajectories and Gravitational Waveforms
• The detectability of eccentric compact binary coalescences with advanced gravitational-wave detectors
• The Eccentric Behavior of Inspiraling Compact Binaries
• Sensitivity functions for space-borne gravitational wave detectors
• Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals
• Hereditary Effects in Eccentric Compact Binary Inspirals to Third Post-Newtonian Order
• Sub-threshold binary neutron star search in Advanced LIGO's first observing run
• Gravitational wave source localization for eccentric binary coalesce with a ground-based detector network
• Potential Gravitational-wave and Gamma-ray Multi-messenger Candidate from Oct. 30, 2015
• Can we Detect Intermediate Mass Ratio Inspirals?
• Convergence of Fourier-domain templates for inspiraling eccentric compact binaries
• Have hierarchical three-body mergers been detected by LIGO/Virgo?
• Improved Constraints on Modified Gravity with Eccentric Gravitational Waves
• Analytic Waveforms for Eccentric Gravitational Wave Bursts
• Excitation of high frequency voices from intermediate-mass-ratio inspirals with large eccentricity
• The Origin of Binary Black Holes Mergers

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• Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
• Spin effects in gravitational waveforms and fluxes for binaries on eccentric orbits to the third post-Newtonian order
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• Unveiling the merger structure of black hole binaries in generic planar orbits
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Defining eccentricity for spin-precessing binaries
• Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Peaking into the abyss: Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes
• False positives for gravitational lensing: the gravitational-wave perspective
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates