activity
20142025
most citedConstraints on a Bianchi type I spacetime extension of the standard CDM model

121 citations · 218 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.CO202315 cited

CDM model: A promising scenario for alleviation of cosmological tensions

Ozgur Akarsu, Eleonora Di Valentino, Suresh Kumar +3

We present a comprehensive analysis of the CDM model, which explores the recent conjecture suggesting a rapid transition of the Universe from anti-de Sitter vacua to de…

gr-qc202319 cited

Cosmological models in scale-independent energy-momentum squared gravity

Ozgur Akarsu, N. Merve Uzun

Scale-independent EMSG is a particular model of energy-momentum squared gravity (EMSG) in which the new terms in the Einstein field equations arising from the EMSG theory enter wit…

gr-qc20215 cited

CDM cosmology with a quiescent anisotropy in a higher dimensional steady state universe

Ozgur Akarsu, Tekin Dereli, Nihan Katirci

In this work, which follows a series of studies on the higher-dimensional steady state universe idea and prepared for Professor Tekin Dereli's Festschrift, we show the influence of…

astro-ph.CO2019121 cited

Constraints on a Bianchi type I spacetime extension of the standard CDM model

Ozgur Akarsu, Suresh Kumar, Shivani Sharma +1

We consider the simplest anisotropic generalization, as a correction, to the standard CDM model, by replacing the spatially flat Robertson-Walker metric by the Bianchi type-I me…

astro-ph.CO201526 cited

A divergence-free parametrization for dynamical dark energy

Ozgur Akarsu, Tekin Dereli, J. Alberto Vazquez

We introduce a new parametrization for the dark energy, led by the same idea to the linear expansion of the equation of state in scale factor and in redshift , which diverge…

gr-qc20144 cited

Accelerated expansion of the Universe a la the Stueckelberg mechanism

Ozgur Akarsu, Metin Arik, Nihan Katirci +1

We investigate a cosmological model in which the Stueckelberg fields are non-minimally coupled to the scalar curvature in a gauge invariant manner. We present not only a solution t…