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

Published 13 Sep 2018 in gr-qc | (1809.05041v1)

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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Authors (1)

Félix-Louis Julié

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