Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe

Based on Tsallis holographic dark energy model recently proposed by using the general model of the Tsallis entropy expression, we reconstruct cosmographic parameters, q,j,κ,l, and we study their evolution in spatially flat (n+1)-dimensional Friedmann-Robertson-Walker universe using Granda-Oliveros s...

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Main Author: Ayman A. Aly
Format: Article
Language:English
Published: Wiley 2019-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2019/8138067
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author Ayman A. Aly
author_facet Ayman A. Aly
author_sort Ayman A. Aly
collection DOAJ
description Based on Tsallis holographic dark energy model recently proposed by using the general model of the Tsallis entropy expression, we reconstruct cosmographic parameters, q,j,κ,l, and we study their evolution in spatially flat (n+1)-dimensional Friedmann-Robertson-Walker universe using Granda-Oliveros scale. Our results show that the universe is in an accelerating expansion mode described by phantom-like behavior. We go further and study the state finder operators and the Om diagnostic to understand the behavior of our model. The stability of the system is also studied by using the square of speed of sound showing that our model is stable over the low range of red-shift considered. The results indicate that the entropy formalism will play an important role in understanding the dynamics of our universe.
format Article
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series Advances in Astronomy
spelling doaj-art-48dd508532be4841a10075e92ab606522025-02-03T05:59:38ZengWileyAdvances in Astronomy1687-79691687-79772019-01-01201910.1155/2019/81380678138067Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW UniverseAyman A. Aly0Physics Department, Faculty of Science, Damanhour University, Damanhour, EgyptBased on Tsallis holographic dark energy model recently proposed by using the general model of the Tsallis entropy expression, we reconstruct cosmographic parameters, q,j,κ,l, and we study their evolution in spatially flat (n+1)-dimensional Friedmann-Robertson-Walker universe using Granda-Oliveros scale. Our results show that the universe is in an accelerating expansion mode described by phantom-like behavior. We go further and study the state finder operators and the Om diagnostic to understand the behavior of our model. The stability of the system is also studied by using the square of speed of sound showing that our model is stable over the low range of red-shift considered. The results indicate that the entropy formalism will play an important role in understanding the dynamics of our universe.http://dx.doi.org/10.1155/2019/8138067
spellingShingle Ayman A. Aly
Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
Advances in Astronomy
title Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
title_full Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
title_fullStr Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
title_full_unstemmed Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
title_short Tsallis Holographic Dark Energy with Granda-Oliveros Scale in (n+1)-Dimensional FRW Universe
title_sort tsallis holographic dark energy with granda oliveros scale in n 1 dimensional frw universe
url http://dx.doi.org/10.1155/2019/8138067
work_keys_str_mv AT aymanaaly tsallisholographicdarkenergywithgrandaoliverosscaleinn1dimensionalfrwuniverse