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Utilizing publicly available non-spinning eccentric binary black hole (BBH) merger simulations (\href{https://data.black-holes.org/waveforms/catalog.html}{https://data.black-holes.org/waveforms/catalog.html}) from the SXS collaboration~\cite{Hinder:2017sxy}, we present convincing evidence that the waveform phenomenology in eccentric BBH mergers is significantly simpler than previously thought.
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Thibault Damour, Achamveedu Gopakumar, and Bala R. Iyer, “Phasing of gravitational waves from inspiralling eccentric binaries,” Phys. Rev. D 70
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Raoul-Martin Memmesheimer, Achamveedu Gopakumar, and Gerhard Schaefer, “Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits,” Phys. Rev. D 70
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Christian Konigsdorffer and Achamveedu Gopakumar, “Phasing of gravitational waves from inspiralling eccentric binaries at the third-and-a-half post-Newtonian order,” Phys. Rev. D 73
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Johan Samsing, “Eccentric Black Hole Mergers Forming in Globular Clusters,” Phys. Rev. D 97
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