Approximate waveform templates for detection of extreme mass ratio inspirals with LISA
Jonathan R Gair

TL;DR
This paper discusses the development of approximate 'kludge' waveforms for detecting extreme mass ratio inspirals with LISA, balancing computational efficiency with waveform fidelity.
Contribution
It introduces the 'numerical kludge' waveform family, outlining its accuracy and potential improvements for efficient EMRI detection.
Findings
The numerical kludge captures main features of true EMRI waveforms.
Approximate waveforms are computationally cheaper and suitable for initial detection.
Potential pathways for improving waveform accuracy are discussed.
Abstract
The inspirals of compact objects into massive black holes are some of the most exciting of the potential sources of gravitational waves for the planned Laser Interferometer Space Antenna (LISA). Observations of such extreme mass ratio inspirals (EMRIs) will not only reveal to us the properties of black holes in the Universe, but will allow us to verify that the space-time structure around massive compact objects agrees with the predictions of relativity. Detection of EMRI signals via matched filtering and interpretation of the observations will require models of the gravitational waveforms. The extreme mass ratio allows accurate waveforms to be computed from black hole perturbation theory, but this is computationally expensive and has not yet been fully developed. Ongoing research to scope out LISA data analysis algorithms requires waveforms that can be generated quickly in large…
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