Note on Tsallis holographic dark energy

Abstract We explore the effects of considering various infrared (IR) cutoffs, including the particle horizon, the Ricci horizon and the Granda–Oliveros (GO) cutoffs, on the properties of Tsallis holographic dark energy (THDE) model, proposed inspired by Tsallis generalized entropy formalism (Tavayef...

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Main Authors: M. Abdollahi Zadeh, A. Sheykhi, H. Moradpour, Kazuharu Bamba
Format: Article
Language:English
Published: SpringerOpen 2018-11-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6427-3
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spelling doaj-8d96677f607e4c80b1e9b2d8ab48ec752020-11-25T00:52:55ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-11-01781111110.1140/epjc/s10052-018-6427-3Note on Tsallis holographic dark energyM. Abdollahi Zadeh0A. Sheykhi1H. Moradpour2Kazuharu Bamba3Physics Department and Biruni Observatory, College of Sciences, Shiraz UniversityPhysics Department and Biruni Observatory, College of Sciences, Shiraz UniversityResearch Institute for Astronomy and Astrophysics of Maragha (RIAAM)Division of Human Support System, Faculty of Symbiotic Systems Science, Fukushima UniversityAbstract We explore the effects of considering various infrared (IR) cutoffs, including the particle horizon, the Ricci horizon and the Granda–Oliveros (GO) cutoffs, on the properties of Tsallis holographic dark energy (THDE) model, proposed inspired by Tsallis generalized entropy formalism (Tavayef et al. in Phys Lett B 781:195, 2018). Interestingly enough, we find that for the particle horizon as IR cutoff, the obtained THDE model can describe the late time accelerated universe. This is in contrast to the usual HDE model which cannot lead to an accelerated universe, if one considers the particle horizon as the IR cutoff. We also investigate the cosmological consequences of THDE under the assumption of a mutual interaction between the dark sectors of the Universe. It is shown that the evolution history of the Universe can be described by these IR cutoffs and thus the current cosmic acceleration can also be realized. The sound instability of the THDE models for each cutoff are also explored, separately.http://link.springer.com/article/10.1140/epjc/s10052-018-6427-3
collection DOAJ
language English
format Article
sources DOAJ
author M. Abdollahi Zadeh
A. Sheykhi
H. Moradpour
Kazuharu Bamba
spellingShingle M. Abdollahi Zadeh
A. Sheykhi
H. Moradpour
Kazuharu Bamba
Note on Tsallis holographic dark energy
European Physical Journal C: Particles and Fields
author_facet M. Abdollahi Zadeh
A. Sheykhi
H. Moradpour
Kazuharu Bamba
author_sort M. Abdollahi Zadeh
title Note on Tsallis holographic dark energy
title_short Note on Tsallis holographic dark energy
title_full Note on Tsallis holographic dark energy
title_fullStr Note on Tsallis holographic dark energy
title_full_unstemmed Note on Tsallis holographic dark energy
title_sort note on tsallis holographic dark energy
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2018-11-01
description Abstract We explore the effects of considering various infrared (IR) cutoffs, including the particle horizon, the Ricci horizon and the Granda–Oliveros (GO) cutoffs, on the properties of Tsallis holographic dark energy (THDE) model, proposed inspired by Tsallis generalized entropy formalism (Tavayef et al. in Phys Lett B 781:195, 2018). Interestingly enough, we find that for the particle horizon as IR cutoff, the obtained THDE model can describe the late time accelerated universe. This is in contrast to the usual HDE model which cannot lead to an accelerated universe, if one considers the particle horizon as the IR cutoff. We also investigate the cosmological consequences of THDE under the assumption of a mutual interaction between the dark sectors of the Universe. It is shown that the evolution history of the Universe can be described by these IR cutoffs and thus the current cosmic acceleration can also be realized. The sound instability of the THDE models for each cutoff are also explored, separately.
url http://link.springer.com/article/10.1140/epjc/s10052-018-6427-3
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