We derive the energy fluxes radiated by compact binary systems, including "hairy" black holes, in Einstein-Maxwell-dilaton theories, for circular orbits and at quadrupolar order. This enables to include in their resummed effective-one-body (EOB) dynamics the effect of the radiation reaction force at the origin of their inspiral and merger. We also exhibit typical examples of the resulting tensor and scalar waveforms.
@article{arxiv.1809.05041,
title = {Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories},
author = {Félix-Louis Julié},
journal= {arXiv preprint arXiv:1809.05041},
year = {2018}
}