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In this paper we develop a waveform model that accurately reproduces thedynamical evolution of intermediate-mass-ratio inspirals, as predicted by theeffective-one-body (EOB) model introduced in [1], and which enables us to shedsome light on the form of the self-force for events with mass-ratio 1:6, 1:10and 1:100. To complement this study, we make use of self-force results in theextreme-mass-ratio regime, and of predictions of the EOB model introduced in[1], to derive a prescription for the shift of the orbital frequency at theinnermost stable circular orbit which consistently captures predictions fromthe extreme, intermediate and comparable mass-ratio regimes.

Accurate modeling of intermediate-mass-ratio inspirals: Exploring the form of the self-force in the intermediate-mass-ratio regime