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• W2776994652 abstract "In modified gravity the propagation of gravitational waves (GWs) is in general different from that in general relativity. As a result, the luminosity distance for GWs can differ from that for electromagnetic signals, and is affected both by the dark energy equation of state $w_{rm DE}(z)$ and by a function $delta(z)$ describing modified propagation. We show that the effect of modified propagation in general dominates over the effect of the dark energy equation of state, making it easier to distinguish a modified gravity model from $Lambda$CDM. We illustrate this using a nonlocal modification of gravity, that has been shown to fit remarkably well CMB, SNe, BAO and structure formation data, and we discuss the prospects for distinguishing nonlocal gravity from $Lambda$CDM with the Einstein Telescope. We find that, depending on the exact sensitivity, a few tens of standard sirens with measured redshift at $zsim 0.4$, or a few hundreds at $1 < z < 2$, could suffice." @default.
• W2776994652 created "2018-01-05" @default.
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• W2776994652 date "2018-05-31" @default.
• W2776994652 modified "2023-10-15" @default.
• W2776994652 title "Gravitational-wave luminosity distance in modified gravity theories" @default.
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• W2776994652 doi "https://doi.org/10.1103/physrevd.97.104066" @default.
• W2776994652 hasPublicationYear "2018" @default.
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