Highly eccentric EMRI waveforms via fast self-forced inspirals
Jonathan McCart, Thomas Osburn, Justin Y. J. Burton

TL;DR
This paper develops and compares new models for highly eccentric EMRI and IMRI inspirals, introducing a fast NIT method for inspiral computation and connecting it to waveform generation, with implications for LISA data analysis.
Contribution
It presents the first application of the near-identity transform to rapidly compute highly eccentric self-forced inspirals and compares waveform models including Teukolsky and kludge approaches.
Findings
NIT inspirals are consistent with full self-force inspirals for EMRIs.
NIT method struggles to meet LISA accuracy goals for highly eccentric IMRIs.
Kludge waveforms compare favorably to Teukolsky waveforms assuming identical worldlines.
Abstract
We present new developments and comparisons of competing inspiral and waveform models for highly eccentric non-spinning extreme and intermediate mass-ratio inspirals (EMRIs and IMRIs). Starting from our high eccentricity self-force library, we apply the near-identity transform (NIT) technique to rapidly compute highly eccentric self-forced inspirals for the first time. Upon evaluating our approximate NIT results via comparison with full self-force inspirals, we couple our accurate and streamlined inspiral data to potential waveform generation schemes. We find that, although high eccentricity strains the NIT method, NIT inspirals are consistent with full self-force inspirals for EMRIs. However, our NIT implementation (at 1st post-adiabatic order) is not able to achieve LISA-motivated accuracy goals for highly eccentric IMRIs. Our most sophisticated waveforms are devised through a new…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Pulsars and Gravitational Waves Research
