Kaluza-Kelin Higher Derivative Gravity and Friedmann-Robertson-Walker Cosmology

TL;DR

This paper derives a compact Friedmann equation in higher-dimensional Kaluza-Klein cosmology, analyzes redundancies in field equations, and explores effects of higher-derivative terms and inflationary solutions.

Contribution

It provides a simplified expression for Friedmann equations in higher dimensions and examines the impact of higher-derivative gravity and inflationary models.

Findings

Higher-order terms do not affect the Friedmann equation in flat internal space.

The derived equations are consistent with Bianchi identities.

Inflationary solutions are discussed within an induced-gravity framework.

Abstract

Kaluza-Klein approach in an N(=1+3+D)-dimensional Friedmann-Robertson-Walker type space is often adopted in the literature. We derive a compact expression for the Friedmann equation in a (1+3+D)-dimensional space. The redundancy of the associated field equations due to the Bianchi identity is analyzed. We also study the dilaton gravity theory with higher-derivative gravitational couplings. It turns out that higher-order terms will not affect the Friedmann equation in a constant flat internal space. This is true only for the flat-De Sitter external space. The inflationary solution in an induced-gravity model is also discussed as an application.