Formation of the large-scale structure of the Universe
V. N. Lukash, E. V. Mikheeva, A. M. Malinovsky
TL;DR
This review discusses how the large-scale structure of the Universe forms, evolves, and decays, integrating observational data, simulations, and the Cosmological Standard Model to address key cosmological questions.
Contribution
It provides a comprehensive overview of the current understanding and challenges in modeling the Universe's large-scale structure within the CSM framework.
Findings
Highlights challenges in measuring cosmological parameters
Discusses methods for determining matter composition
Addresses issues in normalizing density perturbation spectra
Abstract
In this review, the formation, evolution, and decay of the large-scale structure of the Universe is discussed in the context of observational data, numerical simulations, and the Cosmological Standard Model (CSM). Problems concerning measuring and interpreting cosmological parameters, determining the composition of matter, and normalizing density perturbation spectra are especially highlighted.
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