Gravitational waves and geometrical optics in scalar-tensor theories
Alice Garoffolo, Gianmassimo Tasinato, Carmelita Carbone, Daniele, Bertacca, Sabino Matarrese

TL;DR
This paper develops a framework within scalar-tensor theories to analyze how gravitational waves propagate through perturbed cosmological space-times, providing tools to test deviations from General Relativity using GW observations.
Contribution
It introduces generalized evolution equations for GW amplitude and polarization in scalar-tensor theories, including effects of non-minimal couplings and cosmological perturbations.
Findings
Derived modified formulas for GW luminosity distance.
Identified conditions for polarization tensor parallel transport.
Analyzed effects of scalar-tensor couplings on GW propagation.
Abstract
The detection of gravitational waves (GWs) propagating through cosmic structures can provide invaluable information on the geometry and content of our Universe, as well as on the fundamental theory of gravity. In order to test possible departures from General Relativity, it is essential to analyse, in a modified gravity setting, how GWs propagate through a perturbed cosmological space-time. Working within the framework of geometrical optics, we develop tools to address this topic for a broad class of scalar-tensor theories, including scenarios with non-minimal, derivative couplings between scalar and tensor modes. We determine the corresponding evolution equations for the GW amplitude and polarization tensor. The former satisfies a generalised evolution equation that includes possible effects due to a variation of the effective Planck scale; the latter can fail to be parallely…
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