Pure geometric $f(R)$ branes

Fuente: arXiv
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Main Authors: Guo, Heng, Wang, Cai-Ling, Lu, Yong-Tao, Sun, Yue, Wang, Lang-Lang
Format: Preprint
Published: 2024
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author Guo, Heng
Wang, Cai-Ling
Lu, Yong-Tao
Sun, Yue
Wang, Lang-Lang
author_facet Guo, Heng
Wang, Cai-Ling
Lu, Yong-Tao
Sun, Yue
Wang, Lang-Lang
contents In this paper, we investigate pure geometric $f(R)$ cosmology branes embedded in five-dimensional spacetime. The form of $f(R)$ is chosen as a polynomial. The Five-dimensional scalar curvature $R$ is assumed to be constant. Based on the value of the four-dimensional cosmological constant $λ_4$, the branes can be classified into Minkowski, de Sitter, and de anti-de Sitter cases. Solutions for each case can be calculated. These solutions are stable against linear tensor perturbations in all cases. In the Minkowski brane case, the zero mode of gravity can be localized on the brane. In the de Sitter brane case, the zero mode and one massive Kaluza-Klein mode can be localized on the brane. In the anti-de Sitter brane case, all massive Kaluza-Klein modes can be localized on the brane. The results of the analysis of tensor fluctuations are the same in both the Einstein frame and the Jordan frame.
format Preprint
id arxiv_https___arxiv_org_abs_2410_11310
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Pure geometric $f(R)$ branes
Guo, Heng
Wang, Cai-Ling
Lu, Yong-Tao
Sun, Yue
Wang, Lang-Lang
High Energy Physics - Theory
General Relativity and Quantum Cosmology
In this paper, we investigate pure geometric $f(R)$ cosmology branes embedded in five-dimensional spacetime. The form of $f(R)$ is chosen as a polynomial. The Five-dimensional scalar curvature $R$ is assumed to be constant. Based on the value of the four-dimensional cosmological constant $λ_4$, the branes can be classified into Minkowski, de Sitter, and de anti-de Sitter cases. Solutions for each case can be calculated. These solutions are stable against linear tensor perturbations in all cases. In the Minkowski brane case, the zero mode of gravity can be localized on the brane. In the de Sitter brane case, the zero mode and one massive Kaluza-Klein mode can be localized on the brane. In the anti-de Sitter brane case, all massive Kaluza-Klein modes can be localized on the brane. The results of the analysis of tensor fluctuations are the same in both the Einstein frame and the Jordan frame.
title Pure geometric $f(R)$ branes
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2410.11310