Relativistic numerical cosmology with Silent Universes
Krzysztof Bolejko

TL;DR
This paper introduces simsilun, a code based on the Silent Universe approach, to simulate relativistic cosmological evolution, revealing nonlinear effects like spatial curvature emergence in large-scale structure formation.
Contribution
It presents the implementation of the Silent Universe equations in a new simulation code and demonstrates its application to Millennium simulation initial conditions.
Findings
Spatial curvature evolves from zero to about 0.1 by present day.
Mean evolution initially follows the ΛCDM model.
Nonlinear structure formation affects cosmological parameters.
Abstract
Relativistic numerical cosmology is most often based either on the exact solutions of the Einstein equations, or perturbation theory, or weak-field limit, or the BSSN formalism. The Silent Universe provides an alternative approach to investigate relativistic evolution of cosmological systems. The silent universe is based on the solution of the Einstein equations in 1+3 comoving coordinates with additional constraints imposed. These constraints include: the gravitational field is sourced by dust and cosmological constant only, both rotation and magnetic part of the Weyl tensor vanish, and the shear is diagnosable. This paper describes the code simsilun (free software distributed under the terms of the reposi General Public License), which implements the equations of the Silent Universe. The paper also discusses applications of the Silent Universe and it uses the Millennium simulation to…
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