In the first part of this work we review the equations of motion for the brane presented in
Friedmann–Robertson–Walker (FRW) form, when the bulk is five-dimensional (A) dS Black …

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 …

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 …

In this paper we first obtain Friedmann equations for the (n− 1)-dimensional brane
embedded in the (n+ 1)-dimensional bulk, with intrinsic curvature term of the brane included …

We disclose a deep connection between thermodynamics and gravity in a general
braneworld model with curvature correction terms on the brane and in the bulk, respectively …

We study the entropy of a FRW universe filled with dark energy (cosmological constant,
quintessence, or phantom). For the general or time-dependent equation of state p= w ρ the …

Non-extensive Tsallis thermostatistics is a widespread paradigm to describe large-scale
gravitational systems. In this work we use Tsallis Cosmology to study thermodynamic gravity …

As soon as an interaction between holographic dark energy and dark matter is taken into
account, the identification of an IR cutoff with the Hubble radius H− 1, in a flat universe, can …

In this paper we employ a recent proposal of C. Tsallis and formulate the first law of
thermodynamics for gravitating systems in terms of the extensive but non-additive entropy …

Several observational constraints are imposed on the interacting holographic model of dark
energy and dark matter. First we use the age parameter today, as given by the WMAP …