most citedInflation via logarithmic entropy-corrected holographic dark energy model

3 citations · 4 across the 3 of their papers we have counts for

collaborators

7 papers

gr-qc2023

- inflation: Sourced by energy-momentum squared gravity

Seyed Ali Hosseini Mansoori, Fereshteh Felegary, Mahmood Roshan +2

In this paper, we examine chaotic inflation within the context of the energy-momentum squared gravity (EMSG) focusing on the energy-momentum powered gravity (EMPG) that incorporate…

astro-ph.CO2023★ 1 cited

Nonperturbative collapse models for collisionless self-gravitating flows

Niels Fardeau, Thomas Buchert, Fosca Al Roumi +1

Structure formation in the Universe has been well-studied within the Eulerian and Lagrangian perturbation theories, where the latter performs substantially better in comparison wit…

gr-qc2016

Interacting Holographic Dark Energy model in Brans-Dicke cosmology and coincidence problem

F. Felegary, F. Darabi, M. R. Setare

We study the dynamics of interacting holographic dark energy model in Brans-Dicke cosmology for the future event horizon and the Hubble horizon cut-offs. We determine the system of…

gr-qc2016★ 3 cited

Inflation via logarithmic entropy-corrected holographic dark energy model

F. Darabi, F. Felegary, M. R. Setare

We study the inflation via logarithmic entropy-corrected holographic dark energy LECHDE model with future event horizon, particle horizon and Hubble horizon cut-offs, and compare t…

gr-qc2016

Evolution of spherical overdensities in new agegraphic dark energy model

M. R. Setare, F. Felegary, F. Darabi

We study the structure formation by investigating the spherical collapse model in the context of new agegraphic dark energy model in flat FRW cosmology. We compute the perturbation…

gr-qc2016

Evolution of spherical over-densities in tachyon scalar field model

M. R. Setare, F. Felegary, F. Darabi

We study the tachyon scalar field model in flat FRW cosmology with the particular potential and the scale factor behavior . We consider the spherical collapse mo…