Screening vs. gevolution: in chase of a perfect cosmological simulation code

DOI10.1016/j.physletb.2022.136911zbMath1486.83003arXiv2106.07638OpenAlexW3172303458MaRDI QIDQ2076688

A. Emrah Yükselci, Alexander Zhuk, Maxim V. Eingorn

Publication date: 22 February 2022

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2106.07638

zbMATH Keywords

cosmological perturbationslarge-scale structureinhomogeneous universeN-body simulationcosmic screeninggevolution

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Inhomogeneity in solid mechanics (74E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Many-body theory; quantum Hall effect (81V70) Perturbations in context of PDEs (35B20) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (1)

Second-order dust perturbations of the non-flat FLRW model with the positive cosmological constant

Uses Software

• gevolution
• CLASS

Cites Work

• N -body methods for relativistic cosmology
• Physical Foundations of Cosmology
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