Generalized Horndeski-Like Einstein Gauss-Bonnet Inflation with Massless Primordial Gravitons
V.K. Oikonomou, F.P. Fronimos

TL;DR
This paper develops a generalized Einstein-Gauss-Bonnet inflation model with non-minimal couplings, examines its compatibility with gravitational wave speed constraints, and demonstrates its viable inflationary phenomenology under certain conditions.
Contribution
It introduces a novel non-minimally coupled Einstein-Gauss-Bonnet inflation framework with kinetic couplings, analyzing its phenomenology under gravitational wave speed constraints.
Findings
The model can satisfy the GW170817 gravitational wave speed constraint.
Under slow-roll conditions, the framework yields analytical inflationary solutions.
Several models within the framework produce phenomenologically viable inflationary predictions.
Abstract
In this work we shall introduce a theoretical framework comprised by a non-minimal coupled canonical scalar field, a non-minimal coupling to the Gauss-Bonnet invariant and a non-minimal kinetic coupling. This theoretical framework is basically a non-minimally coupled Einstein-Gauss-Bonnet theory with extra corrections of the form of a non-minimal kinetic coupling. In order to comply with the GW170817 event, we shall impose a constraint on the propagation speed of the primordial tensor perturbations that it is equal to that of light's in vacuum, and this constraint basically specifies the way that the scalar potential and the non-minimal couplings of the theory can be chosen. The whole theoretical framework, which belongs to the larger class of Horndeski theories, cannot yield viable results, due to the fact that the primordial gravitational wave speed is not equal to that of light's.…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
