title: Modeling extreme mass ratio inspirals within the effective-one-body approach.
abstract: We present the first models of extreme-mass-ratio inspirals within the effective-one-body (EOB) formalism, focusing on quasicircular orbits into nonrotating black holes. We show that the phase difference and (Newtonian-normalized) amplitude difference between analytical EOB and numerical Teukolsky-based gravitational waveforms can be reduced to less than or approximately 10{-1} rad and less than or approximately 2x10{-3}, respectively, after a 2-year evolution. The inclusion of post-Newtonian self-force terms in the EOB approach leads to a phase disagreement of approximately 6-27 rad after a 2-year evolution. Such inclusion could also allow for the EOB modeling of waveforms from intermediate-mass-ratio, quasicircular inspirals.
authors.affiliation: Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
authors.forename: Nicolás
authors.initials: N
authors.lastname: Yunes
authors.forename: Alessandra
authors.initials: A
authors.lastname: Buonanno
authors.forename: Scott A
authors.initials: SA
authors.lastname: Hughes
authors.forename: M Coleman
authors.initials: MC
authors.lastname: Miller
authors.forename: Yi
authors.initials: Y
authors.lastname: Pan