Tsallis holographic dark energy in Bianchi type–II, VIII and IX universes

Santhi, M. Vijaya; Chinnappalanaidu, T.

doi:10.1007/s10509-023-04189-z

Astrophys Space Sci

2023

DOI: 10.1007/s10509-023-04189-z

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Tsallis holographic dark energy in Bianchi type–II, VIII and IX universes

M. Vijaya Santhi

T. Chinnappalanaidu

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2024

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Cited by 1 publication

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Barrow holographic dark energy: reconstruction within Saez-Ballester theory in Kantowski-Sachs universe

Chokyi,

Chattopadhyay,

Tawfik

2024

Phys. Scr.

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Within the framework of the Saez-Ballester theory, the Barrow Holographic Dark Energy (BHDE) has been reconstructed. This reconstruction was carried out in a homogeneous and anisotropic KS universe that was filled with BHDE. The study examined both non-interacting and interacting scenarios, with the future event horizon serving as the IR cut-off. The analysis focused on the evolution of the Equation of State parameter for both cases, as well as the trajectories of $w_{DE}-w'_{DE}$. Additionally, the study investigated the inflation of the universe filled with BHDE by plotting the slow-roll parameters. Furthermore, a connection between the canonical scalar field and BHDE was explored, as the presence of a scalar field is often associated with inflation. Finally, the tensor-to-scalar ratio $r$ is plotted which seems to lie within the acceptable range.

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Barrow holographic dark energy: reconstruction within Saez-Ballester theory in Kantowski-Sachs universe

Chokyi,

Chattopadhyay,

Tawfik

2024

Phys. Scr.

View full text Add to dashboard Cite

show abstract

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Tsallis holographic dark energy in Bianchi type–II, VIII and IX universes

Cited by 1 publication

References 112 publications

Barrow holographic dark energy: reconstruction within Saez-Ballester theory in Kantowski-Sachs universe

Barrow holographic dark energy: reconstruction within Saez-Ballester theory in Kantowski-Sachs universe

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