Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction

Abstract In this work devoted to the investigation of the Tsallis holographic dark energy (IR cut-off is Hubble radius) in homogeneous and anisotropic Kantowski–Sachs Universe within the frame-work of Saez–Ballester scalar tensor theory of gravitation. We have constructed non-interacting and interac...

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Autores principales: Y. Sobhanbabu, M. Vijaya Santhi
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Publicado: SpringerOpen 2021
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Acceso en línea:https://doaj.org/article/f1adf70f90d74f3695459db28b7980bf
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spelling oai:doaj.org-article:f1adf70f90d74f3695459db28b7980bf2021-11-28T12:11:52ZKantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction10.1140/epjc/s10052-021-09815-01434-60441434-6052https://doaj.org/article/f1adf70f90d74f3695459db28b7980bf2021-11-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09815-0https://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract In this work devoted to the investigation of the Tsallis holographic dark energy (IR cut-off is Hubble radius) in homogeneous and anisotropic Kantowski–Sachs Universe within the frame-work of Saez–Ballester scalar tensor theory of gravitation. We have constructed non-interacting and interacting Tsallis holographic dark energy models by solving the field equations using the relationship between the metric potentials. This relation leads to a viable deceleration parameter model which exhibits a transition of the Universe from deceleration to acceleration. In interacting case, we focus on sign-changeable interaction between Tsallis holographic dark energy and dark matter. The dynamical parameters like equation of state parameter, energy densities of Tsallis holographic dark energy and dark matter, deceleration parameter, and statefinder parameters of the models are explained through graphical representation. And also, we discussed the stability analysis of the our models.Y. SobhanbabuM. Vijaya SanthiSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 11, Pp 1-10 (2021)
institution DOAJ
collection DOAJ
language EN
topic Astrophysics
QB460-466
Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
spellingShingle Astrophysics
QB460-466
Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
Y. Sobhanbabu
M. Vijaya Santhi
Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
description Abstract In this work devoted to the investigation of the Tsallis holographic dark energy (IR cut-off is Hubble radius) in homogeneous and anisotropic Kantowski–Sachs Universe within the frame-work of Saez–Ballester scalar tensor theory of gravitation. We have constructed non-interacting and interacting Tsallis holographic dark energy models by solving the field equations using the relationship between the metric potentials. This relation leads to a viable deceleration parameter model which exhibits a transition of the Universe from deceleration to acceleration. In interacting case, we focus on sign-changeable interaction between Tsallis holographic dark energy and dark matter. The dynamical parameters like equation of state parameter, energy densities of Tsallis holographic dark energy and dark matter, deceleration parameter, and statefinder parameters of the models are explained through graphical representation. And also, we discussed the stability analysis of the our models.
format article
author Y. Sobhanbabu
M. Vijaya Santhi
author_facet Y. Sobhanbabu
M. Vijaya Santhi
author_sort Y. Sobhanbabu
title Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
title_short Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
title_full Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
title_fullStr Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
title_full_unstemmed Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction
title_sort kantowski–sachs tsallis holographic dark energy model with sign-changeable interaction
publisher SpringerOpen
publishDate 2021
url https://doaj.org/article/f1adf70f90d74f3695459db28b7980bf
work_keys_str_mv AT ysobhanbabu kantowskisachstsallisholographicdarkenergymodelwithsignchangeableinteraction
AT mvijayasanthi kantowskisachstsallisholographicdarkenergymodelwithsignchangeableinteraction
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