output
20182024
most citedScalar perturbations in gravity using the covariant approach

37 citations

11 papers

astro-ph.CO2024

Constraints of Cosmic Expansion Using an MSF

Goratamang Gaedie, Shambel Sahlu, Amare Abebe

In this paper, we propose a modified scale factor (MSF) that allows us to explore the accelerating expansion of the universe without invoking the traditional dark-energy model, as…

gr-qc2024★ 8 cited

Constraining viscous fluid models in gravity with data

Shambel Sahlu, Renier T. Hough, Amare Abebe +1

We investigate the impact of bulk viscosity on the accelerating expansion and large-scale structure formation of a Universe in which the underlying gravitational interaction is des…

astro-ph.CO2024★ 11 cited

The cosmology of gravity: constraining the background and perturbed dynamics

Shambel Sahlu, Alnadhief H. A. Alfedeel, Amare Abebe

This paper delves into the late-time accelerated expansion of the universe and the evolution of cosmic structures within the context of a specific \( f(R, L_m) \) gravity model, fo…

gr-qc2024★ 19 cited

Structure growth in cosmology

Shambel Sahlu, Álvaro de la Cruz-Dombriz, Amare Abebe

We take into account redshift-space distortion measurements to investigate the growth of cosmological large-scale structures within the framework of modified symmetric teleparallel…

cond-mat.mtrl-sci2023★ 2 cited

The amplitudons of dynamical stable binary cubic crystals for hot-electron cooling in BaTe, CdTe, SrTe and SnTe for enhanced photo voltaic effect

Tewodros Eyob Ada, Kenate Nemera Nigussa, Lemi Demeyu Deja +1

Dynamical properties of materials determined using force constant expansions in the HIPHIVE package and density functional theory as implemented in the Gpaw code. Thermal conductiv…

gr-qc2021

Covariant density and velocity perturbations of the quasi-Newtonian cosmological model in gravity

Heba Sami, Shambel Sahlu, Amare Abebe +1

We investigate classes of shear-free cosmological dust models with irrotational fluid flows within the framework of gravity. In particular, we use the covariant form…