Disformal invariance of cosmological perturbations in a generalized class of Horndeski theories
Shinji Tsujikawa

TL;DR
This paper demonstrates that cosmological perturbations in a broad class of Horndeski theories remain invariant under disformal transformations, establishing a link between different frames and analyzing implications for inflationary spectra.
Contribution
It proves the invariance of scalar and tensor perturbations under disformal transformations in generalized Horndeski theories using effective field theory methods.
Findings
Cosmological perturbations are invariant under disformal transformations in these theories.
The inflationary power spectra are unchanged up to next-to-leading order in slow-roll.
Conditions for the existence of an Einstein frame with standard tensor spectrum are derived.
Abstract
It is known that Horndeski theories can be transformed to a sub-class of Gleyzes-Langlois-Piazza-Vernizzi (GLPV) theories under the disformal transformation of the metric , where is a function of a scalar field and is another function depending on both and . We show that, with the choice of unitary gauge, both curvature and tensor perturbations on the flat isotropic cosmological background are generally invariant under the disformal transformation. By means of the effective field theories encompassing Horndeski and GLPV theories, we obtain the second-order actions of scalar/tensor perturbations and present the relations for physical quantities between the two frames. The invariance of the inflationary power…
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