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Main Authors: Mbewe, BG, Mekuria, RR, Sahlu, S, Abebe, A
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2412.02276
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author Mbewe, BG
Mekuria, RR
Sahlu, S
Abebe, A
author_facet Mbewe, BG
Mekuria, RR
Sahlu, S
Abebe, A
contents In this paper, we study the viscous fluid cosmological model that when certain conditions are invoked mimics the $Λ$CDM model. The background equations governing the evolution of viscous interacting fluids in a multifluid system are derived. The Markov Chain Monte Carlo (MCMC) simulation is applied to constrain the best-fit cosmological parameters with Supernova Type 1a data. In addition, linear cosmological perturbations are investigated in a dust-matter-dominated frame using a $1+3$ covariant formalism approach. It is evident from the perturbation results obtained that the model predicts the disintegration of bound structures of large-scale structures in the late-time universe.
format Preprint
id arxiv_https___arxiv_org_abs_2412_02276
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Viscous cosmological fluids and large-scale structure
Mbewe, BG
Mekuria, RR
Sahlu, S
Abebe, A
General Relativity and Quantum Cosmology
In this paper, we study the viscous fluid cosmological model that when certain conditions are invoked mimics the $Λ$CDM model. The background equations governing the evolution of viscous interacting fluids in a multifluid system are derived. The Markov Chain Monte Carlo (MCMC) simulation is applied to constrain the best-fit cosmological parameters with Supernova Type 1a data. In addition, linear cosmological perturbations are investigated in a dust-matter-dominated frame using a $1+3$ covariant formalism approach. It is evident from the perturbation results obtained that the model predicts the disintegration of bound structures of large-scale structures in the late-time universe.
title Viscous cosmological fluids and large-scale structure
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.02276