Fetching the paper…
Reading the bibliography…
The detection of gravitational-wave signals from coalescing eccentric binary black holes would yield unprecedented information about the formation and evolution of compact binaries in specific scenarios, such as dynamical formation in dense stellar clusters and three-body interactions.
The evolution of orbits of artificial satellites of planets under the action of gravitational perturbations of external bodies
Lidov ML · 1962
Earlier work this paper cites.
Gravitational Radiation and the Motion of Two Point Masses
Peters PC · 1964
Earlier work this paper cites.
Smoothing and Differentiation of Data by Simplified Least Squares Procedures
Savitzky A, Golay MJE · 1964
Earlier work this paper cites.
Asteroids with large secular orbital variations
Kozai Y · 1980
Earlier work this paper cites.
Effective one-body approach to general relativistic two-body dynamics
Buonanno A, Damour T · 1999
Earlier work this paper cites.
Orbital eccentricity growth through disc-companion tidal interaction
Papaloizou, J C B , Nelson, R P , Masset, F · 2001
Earlier work this paper cites.
Estellés H, Ramos-Buades A, Husa S, García-Quirós C, Colleoni M, Haegel L, et al.. IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes; 2020 · 2004
Earlier work this paper cites.
American Astronomical Society; 2006
Gultekin K, Miller MC, Hamilton DP. Three-Body Dynamics with Gravitational Wave Emission · 2006
Earlier work this paper cites.
Reducing orbital eccentricity in binary black hole simulations
Pfeiffer HP, Brown DA, Kidder LE, Lindblom L, Lovelace G, Scheel MA · 2007
Earlier work this paper cites.
Gayathri V, Healy J, Lange J, O’Brien B, Szczepanczyk M, Bartos I, et al.. GW190521 as a Highly Eccentric Black Hole Merger; 2020 · 2009
Earlier work this paper cites.
Abbott BP, et al.. GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run; 2020 · 2010
Earlier work this paper cites.
Matching post-Newtonian and numerical relativity waveforms: Systematic errors and a new phenomenological model for nonprecessing black hole binaries
Santamaría L, Ohme F, Ajith P, Brügmann B, Dorband N, Hannam M, et al · 2010
Earlier work this paper cites.
Effective-one-body waveforms calibrated to numerical relativity simulations: Coalescence of nonprecessing, spinning, equal-mass black holes
Pan Y, Buonanno A, Buchman LT, Chu T, Kidder LE, Pfeiffer HP, et al · 2010
Earlier work this paper cites.
Measuring orbital eccentricity and periastron advance in quasicircular black hole simulations
Mroué AH, Pfeiffer HP, Kidder LE, Teukolsky SA · 2010
Earlier work this paper cites.
Ajith P, et al.. Data formats for numerical relativity waves; 2011 · 2011
Earlier work this paper cites.
Gravitational-Wave Tests of General Relativity with Ground-Based Detectors and Pulsar-Timing Arrays
Yunes N, Siemens X · 2013
Earlier work this paper cites.
The formation of eccenric compact binary inspirals and the role of gravitational wave emission in binary-single stellar encounters
Samsing J, MacLeod M, Ramirez-Ruiz E · 2014
Earlier work this paper cites.
Accurate and efficient waveforms for compact binaries on eccentric orbits
Huerta EA, Kumar P, McWilliams ST, O’Shaughnessy R, Yunes N · 2014
Earlier work this paper cites.
Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms
Hannam M, Schmidt P, Bohé A, Haegel L, Husa S, Ohme F, et al · 2014
Earlier work this paper cites.
Effective-one-body model for black-hole binaries with generic mass ratios and spins
Taracchini A, Buonanno A, Pan Y, Hinderer T, Boyle M, Hemberger DA, et al · 2014
Cited alongside, same era.
Characterization of the LIGO detectors during their sixth science run
Aasi J, et al · 2015
Cited alongside, same era.
Advanced Virgo: a second-generation interferometric gravitational wave detector
Acernese F, et al · 2015
Cited alongside, same era.
Frequency and time-domain inspiral templates for comparable mass compact binaries in eccentric orbits
Tanay S, Haney M, Gopakumar A · 2016
Cited alongside, same era.
Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order
Moore B, Favata M, Arun KG, Mishra CK · 2016
Cited alongside, same era.
Frequency-domain gravitational waves from nonprecessing black-hole binaries. II. A phenomenological model for the advanced detector era
Improved constraints on modified gravity with eccentric gravitational waves
Ma S, Yunes N · 2019
Later among the works it cites.
Searching for eccentricity: signatures of dynamical formation in the first gravitational-wave transient catalogue of LIGO and Virgo
Romero-Shaw IM, Lasky PD, Thrane E · 2019
Later among the works it cites.
Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
Khan S, Chatziioannou K, Hannam M, Ohme F · 2019
Later among the works it cites.
Enhancing gravitational waveform models through dynamic calibration
Setyawati Y, Ohme F, Khan S · 2019
Later among the works it cites.
Simple procedures to reduce eccentricity of binary black hole simulations
Ramos-Buades A, Husa S, Pratten G · 2019
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
Khan S, Husa S, Hannam M, Ohme F, Pürrer M, Forteza XJ, et al · 2016
Cited alongside, same era.
https://dcc.ligo.org/LIGO-P1600143/public
”Exploring the Sensitivity of Next Generation Gravitational Wave Detectors”; 2016 · 2016
Cited alongside, same era.
Amaro-Seoane P, et al.. Laser Interferometer Space Antenna; 2017 · 2017
Cited alongside, same era.
Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism
Cao Z, Han WB · 2017
Cited alongside, same era.
Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
Bohé A, Shao L, Taracchini A, Buonanno A, Babak S, Harry IW, et al · 2017
Cited alongside, same era.
Measuring eccentricity in binary black hole inspirals with gravitational waves
Lower ME, Thrane E, Lasky PD, Smith R · 2018
Cited alongside, same era.
Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries
Rodriguez CL, Amaro-Seoane P, Chatterjee S, Kremer K, Rasio FA, Samsing J, et al · 2018
Cited alongside, same era.
Reitze D, et al · 2019
Later among the works it cites.
Faithful analytical effective-one-body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
Chiaramello D, Nagar A · 2020
Later among the works it cites.
On the origin of GW190425
Romero-Shaw IM, Farrow N, Stevenson S, Thrane E, Zhu XJ · 2020
Later among the works it cites.
GW190521: A Binary Black Hole Merger with a Total Mass of 150 M ⨀ 150\text{ }\text{ }{M}_{\bigodot}
Abbott R, et al · 2020
Later among the works it cites.
http://www.black-holes.org/waveforms
”SXS catalog”; 2020 · 2020
Later among the works it cites.
Including higher order multipoles in gravitational-wave models for precessing binary black holes
Khan S, Ohme F, Chatziioannou K, Hannam M · 2020
Later among the works it cites.
Regression methods in waveform modeling: a comparative study
Setyawati Y, Pürrer M, Ohme F · 2020
Later among the works it cites.
Science case for the Einstein telescope
Maggiore M, et al · 2020
Later among the works it cites.
https://arxiv.org/abs/2101.08624
Nagar A, Bonino A, Rettegno P. All in one: effective one body multipolar waveform model for spin-aligned, quasi-circular, eccentric, hyperbolic black hole binaries; 2021 · 2021
Closest in time.
Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: Comparable mass, nonspinning case
Islam T, Varma V, Lodman J, Field SE, Khanna G, Scheel MA, et al · 2021
Closest in time.
Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes
Pratten G, García-Quirós C, Colleoni M, Ramos-Buades A, Estellés H, Mateu-Lucena M, et al · 2021
Closest in time.
Zenodo; 2021
Setyawati Y, Ohme F. Yoshinta/pyrex: public release of pyrex · 2021
Closest in time.
[Online; accessed 20-Jan-2021]
Upgraded LIGO to search for universe’s most extreme events; 2019 · 2021
Closest in time.
GW190521: Orbital Eccentricity and Signatures of Dynamical Formation in a Binary Black Hole Merger Signal
Romero-Shaw I, Lasky PD, Thrane E, Bustillo JC · 2041
Closest in time.