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20092025
most citedFirst-order Cosmological Perturbations Engendered by Point-like Masses

58 citations · 733 across the 70 of their papers we have counts for

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gr-qc2024

A quantitative analysis of the effect of box size in N-body simulations of the matter power spectrum

Maxim Eingorn, Ezgi Yilmaz, A. Emrah Yükselci +1

We study the effect of box size on the matter power spectrum obtained via cosmological N-body simulations. Within the framework of the cosmic screening approach, we show that the r…

gr-qc2023★ 1 cited

Mass density vs. energy density at cosmological scales

Maxim Eingorn, Ezgi Yilmaz, A. Emrah Yükselci +1

In the presence of the gravitational field, the energy density of matter no longer coincides with its mass density. A discrepancy exists, of course, also between the associated pow…

gr-qc2023★ 1 cited

Suppression of matter density growth at scales exceeding the cosmic screening length

Maxim Eingorn, Ezgi Yilmaz, A. Emrah Yükselci +1

One of the main objectives of modern cosmology is to explain the origin and evolution of cosmic structures at different scales. The principal force responsible for the formation of…

gr-qc2023★ 1 cited

Backreaction in cosmic screening approach

Maxim Eingorn, Brianna O'Briant, Adjaratou Diouf +1

We investigate the backreaction of nonlinear perturbations on the global evolution of the Universe within the cosmic screening approach. To this end, we have considered the second-…

gr-qc2022★ 2 cited

Cosmological Perturbations Engendered by Discrete Relativistic Species

Maksym Brilenkov, Ezgi Canay, Maxim Eingorn

Within the extension of the CDM model, allowing for the presence of neutrinos or warm dark matter, we develop the analytical cosmological perturbation theory. It covers all spat…

gr-qc2022★ 1 cited

Effect of peculiar velocities of inhomogeneities on the shape of gravitational potential in spatially curved universe

Ezgi Canay, Maxim Eingorn, Andrew McLaughlin +2

We investigate the effect of peculiar velocities of inhomogeneities and the spatial curvature of the universe on the shape of the gravitational potential. To this end, we consider…