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

Abstract 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 scala...

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Main Authors: P. S. Ens, A. F. Santos
Format: Article
Language:English
Published: SpringerOpen 2024-12-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-024-13708-3
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author P. S. Ens
A. F. Santos
author_facet P. S. Ens
A. F. Santos
author_sort P. S. Ens
collection DOAJ
description Abstract 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 Article
id doaj-art-83e487e6c6444eae8a93bbe34f6ba162
institution Kabale University
issn 1434-6052
language English
publishDate 2024-12-01
publisher SpringerOpen
record_format Article
series European Physical Journal C: Particles and Fields
spelling doaj-art-83e487e6c6444eae8a93bbe34f6ba1622025-02-02T12:39:30ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522024-12-01841211010.1140/epjc/s10052-024-13708-3Barrow holographic dark energy: a path to reconstructing f(R, T) gravityP. S. Ens0A. F. Santos1Programa de Pós-Graduação em Física, Instituto de Física, Universidade Federal de Mato GrossoPrograma de Pós-Graduação em Física, Instituto de Física, Universidade Federal de Mato GrossoAbstract 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.https://doi.org/10.1140/epjc/s10052-024-13708-3
spellingShingle P. S. Ens
A. F. Santos
Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
European Physical Journal C: Particles and Fields
title Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
title_full Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
title_fullStr Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
title_full_unstemmed Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
title_short Barrow holographic dark energy: a path to reconstructing f(R, T) gravity
title_sort barrow holographic dark energy a path to reconstructing f r t gravity
url https://doi.org/10.1140/epjc/s10052-024-13708-3
work_keys_str_mv AT psens barrowholographicdarkenergyapathtoreconstructingfrtgravity
AT afsantos barrowholographicdarkenergyapathtoreconstructingfrtgravity