Strategies for observing extreme mass ratio inspirals

TL;DR

This paper reviews strategies for observing Extreme Mass Ratio Inspirals (EMRIs) with gravitational wave detectors, focusing on waveform modeling, data analysis algorithms, and includes a new estimate for the observational timescale of radiation effects.

Contribution

It provides a comprehensive review of current methods for EMRI observation and introduces a novel analytical estimate for the timescale of negligible radiation influence.

Findings

Waveform generation techniques for EMRIs

Status of data analysis algorithms for EMRI detection

New analytical estimate for radiation influence timescale

Abstract

I review the status of research, conducted by a variety of independent groups, aimed at the eventual observation of Extreme Mass Ratio Inspirals (EMRIs) with gravitational wave detectors. EMRIs are binary systems in which one of the objects is much more massive than the other, and which are in a state of dynamical evolution that is dominated by the effects of gravitational radiation. Although these systems are highly relativistic, with the smaller object moving relative to the larger at nearly light-speed, they are well described by perturbative calculations which exploit the mass ratio as a natural small parameter. I review the use of such approximations to generate waveforms needed by data analysis algorithms for observation. I also briefly review the status of developing the data analysis algorithms themselves. Although this article is almost entirely a review of previous work, it includes (as an appendix) a new analytical estimate for the time over which the influence of radiation on the binary itself is observationally negligible.