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Similar

S. Foffa, M. Maggiore, and E. Mitsou, “Cosmological dynamics and dark energy from non-local infrared modifications of gravity,” Int.J.Mod.Phys
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M. Maggiore, “Nonlocal Infrared Modifications of Gravity. A Review,” Fundam. Theor. Phys
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2019

Nonlocal gravity and gravitational-wave observations

Belgacem, Enis, Dirian, Yves, Finke, Andreas et al.

Understand

We discuss a modified gravity model which fits cosmological observations at a level statistically indistinguishable from $\Lambda$CDM and at the same time predicts very large deviations from General Relativity (GR) in the propagation of gravitational waves (GWs) across cosmological distances.

The model is a variant of the RT nonlocal model proposed and developed by our group, with initial conditions set during inflation, and predicts a GW luminosity distance that, at the redshifts accessible to LISA or to a third-generation GW detector such as the Einstein Telescope (ET), can differ from that in GR by as much as $60\%$.
An effect of this size could be detected with just a single standard siren with counterpart by LISA or ET.
At the redshifts accessible to a LIGO/Virgo/Kagra network at target sensitivity the effect is smaller but still potentially detectable.