Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories

Published 19 October 2018 © 2018 IOP Publishing Ltd and Sissa Medialab
, , Citation Félix-Louis Julié JCAP10(2018)033 DOI 10.1088/1475-7516/2018/10/033

1475-7516/2018/10/033

Abstract

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.

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10.1088/1475-7516/2018/10/033