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Gravitational-wave emission in shift-symmetric Horndeski theories

Gravity theories beyond General Relativity typically predict dipolar gravitational emission by compact-star binaries. This emission is sourced by "sensitivity" parameters depending on the stellar compactness. We introduce a general formalism to calculate these parameters, and show that in shift-symmetric Horndeski theories stellar sensitivities and dipolar radiation vanish, provided that the binary's dynamics is perturbative (i.e. the post-Newtonian formalism is applicable) and cosmological-expansion effects can be neglected. This allows reproducing the binary-pulsar observed orbital decay.

preprint2015arXivOpen access
Enrico BarausseKent Yagi
astro-ph.COgr-qchep-th
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Enrico BarausseKent Yagi

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