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• W2171097706 abstract "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 one to reproduce the binary-pulsar-observed orbital decay." @default.
• W2171097706 created "2016-06-24" @default.
• W2171097706 creator A5049026088 @default.
• W2171097706 creator A5068056500 @default.
• W2171097706 date "2015-11-20" @default.
• W2171097706 modified "2023-10-15" @default.
• W2171097706 title "Gravitation-Wave Emission in Shift-Symmetric Horndeski Theories" @default.
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• W2171097706 doi "https://doi.org/10.1103/physrevlett.115.211105" @default.
• W2171097706 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/26636840" @default.
• W2171097706 hasPublicationYear "2015" @default.
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