Barrow holographic dark energy: a path to reconstructing $f(R,T)$ gravity

Fuente: arXiv
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Auteurs principaux: Ens, P. S., Santos, A. F.
Format: Preprint
Publié: 2024
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author Ens, P. S.
Santos, A. F.
author_facet Ens, P. S.
Santos, A. F.
contents In this paper, we investigate one of the established methods for reconstructing modified gravity models from a dark energy model, with the aim of discovering relationships between these theories. In this study, we focus on the $f(R,T)$ modified gravity theory, where $R$ denotes the Ricci scalar and $T$ represents the trace of the energy-momentum tensor. We employ Barrow's holographic dark energy model, derived from fractal surfaces of black holes, to investigate the reconstruction process. The numerical results are subsequently presented for various infrared cutoffs, such as the Hubble horizon, future event horizon, and Granda-Oliveros cutoff.
format Preprint
id arxiv_https___arxiv_org_abs_2412_09189
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Barrow holographic dark energy: a path to reconstructing $f(R,T)$ gravity
Ens, P. S.
Santos, A. F.
General Relativity and Quantum Cosmology
In this paper, we investigate one of the established methods for reconstructing modified gravity models from a dark energy model, with the aim of discovering relationships between these theories. In this study, we focus on the $f(R,T)$ modified gravity theory, where $R$ denotes the Ricci scalar and $T$ represents the trace of the energy-momentum tensor. We employ Barrow's holographic dark energy model, derived from fractal surfaces of black holes, to investigate the reconstruction process. The numerical results are subsequently presented for various infrared cutoffs, such as the Hubble horizon, future event horizon, and Granda-Oliveros cutoff.
title Barrow holographic dark energy: a path to reconstructing $f(R,T)$ gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.09189