A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
arXiv:2104.03789 · doi:10.1103/PhysRevD.103.124053
Abstract
A waveform model for the eccentric binary black holes named SEOBNRE has been used to analyze the LIGO-Virgo's gravitational wave data by several groups. The accuracy of this model has been validated by comparing it with numerical relativity. However, SEOBNRE is a time-domain model, and the efficiency for generating waveforms is a bottleneck in data analysis. To overcome this disadvantage, we offer a reduced-order surrogate model for eccentric binary black holes based on the SEOBNRE waveforms. This surrogate model (SEOBNRE\_S) can simulate the complete inspiral-merger-ringdown waves with enough accuracy, covering eccentricities from 0 to 0.25 (0.1), and mass ratio from 1:1 to 5:1 (2:1) for nonspinning (spinning) binaries. The speed of waveform generation is accelerated about times than the original SEOBNRE model. Therefore SEOBNRE\_S could be helpful in the analysis of LIGO data to find potential eccentricities.
arXiv comment18pages, 23 figures
References in corpus (89)
- 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
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- Tests of general relativity with GW150914
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- GW190521: A Binary Black Hole Merger with a Total Mass of
- Effective one-body approach to general relativistic two-body dynamics
- Characterization of the LIGO detectors during their sixth science run
- A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- Black hole mergers in the universe
- FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
- A new route towards merging massive black holes
- Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
- Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
- Gravitational waves from scattering of stellar-mass black holes in galactic nuclei
- The dynamical evolution of massive black hole binaries - I. Hardening in a fixed stellar background
- Double Compact Objects III: Gravitational Wave Detection Rates
- Surrogate models for precessing binary black hole simulations with unequal masses
- Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO
- The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
- On the Eccentricity Distribution of Coalescing Black Hole Binaries Driven by the Kozai Mechanism in Globular Clusters
- Binary black hole mergers from field triples: properties, rates and the impact of stellar evolution
- Eccentric Black Hole Mergers Forming in Globular Clusters
- Binary Mergers and Growth of Black Holes in Dense Star Clusters
- Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
- Evolution of Binary Compact Objects Which Merge
- GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal
- Lidov-Kozai Cycles with Gravitational Radiation: Merging Black Holes in Isolated Triple Systems
- Surrogate model of hybridized numerical relativity binary black hole waveforms
- Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
- The LIGO Open Science Center
- Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers
- Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
- Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters
- Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
- Dynamical Formation of the GW150914 Binary Black Hole
- Fast prediction and evaluation of gravitational waveforms using surrogate models
- Black hole triple dynamics: breakdown of the orbit average approximation and implications for gravitational wave detections
- 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
- Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
- Compact Binaries in Star Clusters I - Black Hole Binaries Inside Globular Clusters
- Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation
- Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
- A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
- Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
- The Effect of Starburst Metallicity on Bright X-Ray Binary Formation Pathways
- A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
- Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
- 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
- Three-Body Dynamics with Gravitational Wave Emission
- High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants
- The Total Merger Rate of Compact Object Binaries In The Local Universe
- Measuring eccentricity in binary black hole inspirals with gravitational waves
- Complete waveform model for compact binaries on eccentric orbits
- Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case
- The Role of the Kozai-Lidov Mechanism in Black Hole Binary Mergers in Galactic Centers
- The Formation and Gravitational-Wave Detection of Massive Stellar Black-Hole Binaries
- A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
- Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs
- Circularization and Final Spin in Eccentric Binary Black Hole Inspirals
- Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
- Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
- Foundations of an effective-one-body model for coalescing binaries on eccentric orbits
- Formation pathway of Population III coalescing binary black holes through stable mass transfer
- Observing complete gravitational wave signals from dynamical capture binaries
- On the role of recombination in common-envelope ejections
- Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
- Dynamical Formation of Low-Mass Merging Black Hole Binaries like GW151226
- A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
- Modeling the source of GW150914 with targeted numerical-relativity simulations
- Search for Eccentric Binary Neutron Star Mergers in the first and second observing runs of Advanced LIGO
- Induced Ellipticity for Inspiraling Binary Systems
- Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
- Hierarchical black hole triples in young star clusters: impact of Kozai-Lidov resonance on mergers
- Compact Binaries in Star Clusters II - Escapers and Detection Rates
- A Proposed Search for the Detection of Gravitational Waves from Eccentric Binary Black Holes
- The NINJA-2 project: Detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations
- Can Neutron-Star Mergers Explain the r-process Enrichment in Globular Clusters?
- Formation and Evolution of Binary Neutron Stars
- body dynamics of Intermediate mass-ratio inspirals in globular clusters
- Gravitational Waves from Hierarchical Triple Systems with Kozai-Lidov Oscillation
- On the Common Envelope Efficiency
- Eccentricity distributions of eccentric binary black holes in galactic nuclei
- Dynamical Formation Scenarios for GW190521 and Prospects for Decihertz Gravitational-Wave Astronomy with GW190521-Like Binaries
Cited by in corpus (28)
- Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
- Signs of eccentricity in two gravitational-wave signals may indicate a sub-population of dynamically assembled binary black holes
- Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
- Inferring eccentricity evolution from observations of coalescing binary black holes
- New Avenue for Accurate Analytical Waveforms and Fluxes for Eccentric Compact Binaries
- A Rosetta Stone for eccentric gravitational waveform models
- Strong-field scattering of two spinning black holes: Numerics versus Analytics
- Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
- Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing 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
- Investigating the relation between gravitational wave tests of general relativity
- Upgraded waveform model of eccentric binary black hole based on effective-one-body-numerical-relativity for spin-aligned binary black holes
- Gravitational-wave inference for eccentric binaries: the argument of periapsis
- 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
- Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
- Defining eccentricity for spin-precessing binaries
- Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
- Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
- Biased parameter inference of eccentric, spin-precessing binary black holes
- Probing eccentric higher-order modes through an effective chirp mass model
- Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
- Gravitational waveform model based on photon motion for spinning black holes
- Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
- The next generation: Impact of high-order analytical information on effective one body waveform models for noncircularized, spin-aligned black hole binaries
- EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
- Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
- Exploiting Newton-factorized, 2PN-accurate, waveform multipoles in effective-one-body models for spin-aligned noncircularized binaries
- Assessment of Effective-One-Body Radiation Reactions for Generic Planar Orbits