Straightforward mode hierarchy in eccentric binary black hole mergers and associated waveform model
Tousif Islam

TL;DR
This paper introduces a simplified waveform model for eccentric binary black hole mergers that leverages a universal eccentric modulation, significantly reducing modeling complexity and achieving high accuracy compared to numerical simulations.
Contribution
The authors present a universal eccentric modulation model that converts quasi-circular waveforms into eccentric ones, simplifying the modeling of eccentric BBH mergers.
Findings
Model mismatches are mostly around 10^{-3}
The model is comparable to numerical errors in simulations
The approach reduces complexity by using a single modulation time-series
Abstract
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. We find that the eccentric modulations in the amplitudes, phases, and frequencies in different spherical harmonic modes are all related and can be modeled using a single time series modulation. Using this universal eccentric modulation, we provide a model named \texttt{gwNRHME} to seamlessly convert a multi-modal (i.e with several spherical harmonic modes) quasi-circular waveform into multi-modal eccentric waveform if the quadrupolar eccentric waveform is known. This reduces the modelling…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Fluid Dynamics and Turbulent Flows
