Two-dimensional (bi-)scalar gravities from four-dimensional Horndeski
M. Shams Nejati, M. H. Vahidinia

TL;DR
This paper derives a two-dimensional bi-scalar gravity model from four-dimensional Horndeski theory using Kaluza-Klein reduction, introducing a concise formulation and analyzing perturbations to identify healthy modes.
Contribution
It presents a novel two-dimensional bi-scalar gravity framework from four-dimensional Horndeski theory, including a new identity and perturbation analysis for healthy modes.
Findings
Support for a single healthy propagating mode.
A concise bi-scalar Lagrangian formulation.
Mapping between 2D dilaton gravity and 4D Horndeski theory.
Abstract
We develop a classical two-dimensional bi-scalar gravity based on the Kaluza-Klein reduction applied to the four-dimensional Horndeski theory. One of the scalar fields arises from the original four-dimensional theory, while the extra scalar emerges from the reduction process. We also introduce a two-dimensional bi-scalar identity that allows for a more concise and elegant reformulation of the resulting bi-scalar Lagrangian. Additionally, we study the linear perturbations around a static background to demonstrate that the bi-scalar theory may support a single healthy propagating mode. Furthermore, by restricting the scalar fields, we investigate a general single scalar theory that is identical to the two-dimensional Horndeski theory up to a boundary term. Our results provide a framework to map a generic two-dimensional dilaton gravity into four-dimensional Horndeski theory.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
