We study the cosmological evolution of a nonflat Friedmann-Robertson-Walker Universe
filled by pressureless dark matter and Barrow holographic dark energy (BHDE). The latter is …

Abstract We reconstruct Barrow Holographic Dark Energy (BHDE) within the framework of
Saez–Ballester Scalar Tensor Theory. As a specific background, we consider a …

We consider a nonflat Friedmann–Robertson–Walker universe filled by a pressureless dark
matter and Tsallis holographic dark energy (THDE) whose IR cutoff is the apparent horizon …

Physical limits on the equation-of-state (EoS) parameter of a dark energy component non-
minimally coupled with the dark matter field are examined in light of the second law of …

We propose an approach considering the nonextensive effects in the context of the Verlinde
theory in order to address an extended cosmological model in the context of viscous dark …

Dark matter (DM) as a pressureless perfect fluid provides a good fit of the standard Λ cold
dark matter (ΛCDM) model to the astrophysical and cosmological data. In this paper, we …

The Janis-Newman-Winicour and Papapetrou metrics represent counterparts to the
Schwarzschild black hole with scalar and antiscalar background fields, correspondingly …

The cosmological redshift drift could lead to the next step in high-precision cosmic geometric
observations, becoming a direct and irrefutable test for cosmic acceleration. In order to test …

We investigate the relation between the Friedmann and thermodynamic pressure equations,
through solving the Friedmann and thermodynamic pressure equations simultaneously. Our …

Abstract Using the Hayward–Kodama temperature for the apparent horizon, it is found that
matter content in the Universe is not thermodynamically stable, and the entry to the late …