We review the paradigm of holographic dark energy (HDE), which arises from a theoretical
attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making …

Recently, Barrow argued that quantum-gravitational effects may introduce intricate, fractal
features on the black hole horizon [JD Barrow,, The area of a rough black hole, Phys. Lett. B …

It is shown that the differential form of Friedmann equation of a FRW universe can be
rewritten as the first law of thermodynamics d E= T d S+ W d V at apparent horizon, where …

We propose a new parametrization of dark energy motivated by thermodynamics. To this
aim, we consider Padé polynomials to reconstruct the form of deceleration parameter …

It was shown by Tsallis and Cirto that thermodynamical entropy of a gravitational system
such as black hole must be generalized to the non-additive entropy, which is given by S h= γ …

We investigate the validity of the generalized second law of thermodynamics, applying
Barrow entropy for the horizon entropy. The former arises from the fact that the black-hole …

In this paper, using Barrow entropy, we propose an interacting model of Barrow holographic
dark energy (BHDE). In particular, we study the evolution of a spatially flat FLRW universe …

Barrow proposed that the area law of the entropy associated with a horizon might receive a
“fractal correction” due to quantum gravitational effects—in place of S∝ A, we have instead …

We investigate the validity of the generalized second law of thermodynamics, in the
cosmological scenario where dark energy interacts with both dark matter and radiation …

We investigate the cosmological consequences of the modified Friedmann equations when
the entropy associated with the apparent horizon, given by Barrow entropy, S∼ A 1+ δ/2 …