Strategies for observing extreme mass ratio inspirals

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. Strategies for observing extreme mass ratio inspirals 2 1. EMRIs and IMRIs This article is intended to be a brief review of a variety of works which share a common ultimate goal: the observation of Extreme Mass Ratio Inspirals (EMRIs) with gravitational wave detectors. I assume that the reader is familiar enough with