Viscous cosmological fluids and large-scale structure
Autor: | Mbewe, BG, Mekuria, RR, Sahlu, S, Abebe, A |
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Rok vydání: | 2024 |
Předmět: | |
Zdroj: | SAIP2023 Proceedings |
Druh dokumentu: | Working Paper |
Popis: | In this paper, we study the viscous fluid cosmological model that when certain conditions are invoked mimics the $\Lambda$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. Comment: Published in SAIP2023 Proceedings, South African Institute of Physics |
Databáze: | arXiv |
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