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Article

Physical Acceptability of the Renyi, Tsallis and Sharma-Mittal Holographic Dark Energy Models in the f(T,B) Gravity under Hubble’s Cutoff

1
Department of Mathematics, S.P.M. Science and Gilani Arts and Commerce College, Yavatmal 445301, India
2
Instituto de Astronomia, Geofísicae Ciências Atmosféricas (IAG), Universidade de São Paulo (USP), São Paulo, SP 05508-090, Brazil
3
Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, India
*
Author to whom correspondence should be addressed.
Academic Editors: Eugene Oks and Piero Nicolini
Universe 2021, 7(3), 67; https://doi.org/10.3390/universe7030067
Received: 29 January 2021 / Revised: 9 March 2021 / Accepted: 10 March 2021 / Published: 12 March 2021
(This article belongs to the Special Issue Advances in Understanding Astrophysical and Atomic Phenomena)
In the present article, we investigate the physical acceptability of the spatially homogeneous and isotropic Friedmann–Lemâitre–Robertson–Walker line element filled with two fluids, with the first being pressureless matter and the second being different types of holographic dark energy. This geometric and material content is considered within the gravitational field equations of the f(T,B) (where T is the torsion scalar and the B is the boundary term) gravity in Hubble’s cut-off. The cosmological parameters, such as the Equation of State (EoS) parameter, during the cosmic evolution, are calculated. The models are stable throughout the universe expansion. The region in which the model is presented is dependent on the real parameter δ of holographic dark energies. For all δ4.5, the models vary from ΛCDM era to the quintessence era. View Full-Text
Keywords: Renyi; Tsallis and Sharma–Mittle holographic dark energy models; f(T,B) gravity Renyi; Tsallis and Sharma–Mittle holographic dark energy models; f(T,B) gravity
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MDPI and ACS Style

Shekh, S.H.; Moraes, P.H.R.S.; Sahoo, P.K. Physical Acceptability of the Renyi, Tsallis and Sharma-Mittal Holographic Dark Energy Models in the f(T,B) Gravity under Hubble’s Cutoff. Universe 2021, 7, 67. https://doi.org/10.3390/universe7030067

AMA Style

Shekh SH, Moraes PHRS, Sahoo PK. Physical Acceptability of the Renyi, Tsallis and Sharma-Mittal Holographic Dark Energy Models in the f(T,B) Gravity under Hubble’s Cutoff. Universe. 2021; 7(3):67. https://doi.org/10.3390/universe7030067

Chicago/Turabian Style

Shekh, Salim H., Pedro H.R.S. Moraes, and Pradyumn K. Sahoo. 2021. "Physical Acceptability of the Renyi, Tsallis and Sharma-Mittal Holographic Dark Energy Models in the f(T,B) Gravity under Hubble’s Cutoff" Universe 7, no. 3: 67. https://doi.org/10.3390/universe7030067

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