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Similar

C. Feng, B. Wang, Y. Gong and R. K. Su, Testing the viability of the interacting holographic dark energy model by using combined observational constraints
Original
2007
Cited alongside, same era.
R. G. Cai, A Dark Energy Model Characterized by the Age of the Universe
Original
2007
Cited alongside, same era.
A. A. Mamon, A. Paliathanasis and S. Saha, Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
Original
2007
Cited alongside, same era.
M. R. Setare and E. N. Saridakis, Correspondence between Holographic and Gauss-Bonnet dark energy models
Original
2008
Cited alongside, same era.
E. N. Saridakis, Restoring holographic dark energy in brane cosmology

Then

R. C. G. Landim, Holographic dark energy from minimal supergravity
Original
2016
Later among the works it cites.
A. Pasqua, S. Chattopadhyay and R. Myrzakulov, Power-law entropy-corrected holographic dark energy in Hořava-Lifshitz cosmology with Granda-Oliveros cut-off
Original
2016
Later among the works it cites.
A. Jawad, N. Azhar and S. Rani, Entropy corrected holographic dark energy models in modified gravity
2016
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E. M. C. Abreu, J. Ananias Neto, E. M. Barboza and R. C. Nunes, Jeans instability criterion from the viewpoint of Kaniadakis’ statistics
Original
2016
Later among the works it cites.
R. C. Nunes, E. M. Barboza, Jr., E. M. C. Abreu and J. A. Neto, Probing the cosmological viability of non-gaussian statistics
Original

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2021

Kaniadakis holographic dark energy and cosmology

Drepanou, Niki, Lymperis, Andreas, Saridakis, Emmanuel N. et al.

Understand

We construct a holographic dark energy scenario based on Kaniadakis entropy, which is a generalization of Boltzmann-Gibbs entropy that arises from relativistic statistical theory and is characterized by a single parameter $K$ which quantifies the deviations from standard expressions, and we use the future event horizon as the Infrared cutoff.

We extract the differential equation that determines the evolution of the effective dark energy density parameter, and we provide analytical expressions for the corresponding equation-of-state and deceleration parameters.
We show that the universe exhibits the standard thermal history, with the sequence of matter and dark-energy eras, while the transition to acceleration takes place at $z\approx0.6$.
Concerning the dark-energy equation-of-state parameter we show that it can have a rich behavior, being quintessence-like, phantom-like, or experience the phantom-divide crossing in the past or in the future.