Cosmological models and misunderstandings about them
Andrzej Krasi\'nski

TL;DR
This paper discusses the advantages of inhomogeneous cosmological models over traditional homogeneous models, clarifies misconceptions, and highlights their ability to explain phenomena like anisotropies and redshift drift.
Contribution
It presents the benefits of inhomogeneous models as exact solutions, corrects common misunderstandings, and illustrates their relevance to observable cosmological effects.
Findings
Inhomogeneous models can describe non-repeatable light paths and anisotropies.
Misunderstandings about singularities and deceleration are addressed and corrected.
Inhomogeneous models explain redshift drift and maximum diameter distance phenomena.
Abstract
Advantages of inhomogeneous cosmological models that are exact solutions of Einstein's equations over linearised perturbations of homogeneous models are presented. Examples of effects that can be described in the inhomogeneous ones are given: the non-repeatable light paths, the observed anisotropies in the cosmic microwave background, the redshift drift and the maximum diameter distance. Criticisms of inhomogeneous models that are based on misunderstandings or fallacious reasonings are pointed out and corrected; these include the "weak singularity", the positivity of deceleration "theorem", the "pathology" of redshift behaviour at the "critical point" and the alleged necessity of the bang time to be constant.
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
