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20102024
most citedScale-dependent power spectrum from initial excited-de Sitter modes

23 citations · 149 across the 25 of their papers we have counts for

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Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2024★ 1 cited

A Quadratic Equation of State to Cosmic Acceleration: Entropy Evolution and Phantom Crossing

A. Shahriar, M. Abbasiyan-Motlaq, M. Mohsenzadeh +1

This paper investigates the thermodynamic evolution of the universe within the framework of a quadratic equation of state (EoS). Building upon the basis of the quadratic EoS model,…

astro-ph.CO2023★ 7 cited

A possible role for the merger of clusters/voids in the cosmological expansion

S. Mohammadi, E. Yusofi, M. Mohsenzadeh +1

In this study, we use the merger process of clusters/voids in the role of variable dark energy fluid to alleviate the Hubble tension, which can lead to a balance in the cosmologica…

astro-ph.CO2022★ 1 cited

Cosmological Constant Problem and Tension in Void-dominated Cosmology

E. Yusofi, M. A. Ramzanpour

In this work, we study the cosmological constant problem and Hubble tension in the void-dominated cosmology scenario \cite{Yusofi:2022hgg}. For this goal, we will first consider th…

astro-ph.CO2019★ 11 cited

Surface Tension of Cosmic Voids as a Possible Source for Dark Energy

E. Yusofi, M. Khanpour, B. Khanpour +2

The cosmological constant is estimated by considering the surface tension of supervoids in a void-dominated cosmic fluid by which we can get a possible source of dark energy. Looki…

astro-ph.CO2017★ 2 cited

Gravitational Merging as a Possible Source for the Cosmological Accelerating

Mehrdad Khanpour, Ebrahim Yusofi, Bahman Khanpour

Gravitational merging (or clustering) of cosmic objects is regarded as a possible source of the extra-acceleration of the universe at large scale. The merging/clustering of cosmic…

astro-ph.CO2017

Reconstruction of initial Asymptotic-de Sitter mode in light of the Planck data

Hossein Moshafi, Ata Sojasi, Ebrahim Yusofi +1

The recently relased \emph{Planck} data, emphasize that the background geometry of inflation is not pure de Sitter, but from the slow variation of Hubble parameter during the infla…