The Diffuse Light of the Universe - On the microwave background before and after its discovery: open questions
Jean-Marc Bonnet-Bidaud (Astrophysics Department, French Alternative, Energies, Atomic Energy Commission (CEA), France)

TL;DR
This paper reviews the history, interpretation challenges, and open questions surrounding the Cosmic Microwave Background, questioning its status as definitive evidence of the Big Bang and exploring alternative explanations.
Contribution
It critically examines the assumptions and interpretations of the CMB, highlighting unresolved issues and proposing alternative perspectives within cosmological theories.
Findings
Highlights uncertainties in CMB interpretation
Discusses historical and alternative explanations
Identifies open questions in cosmology
Abstract
In 1965, the discovery of a new type of uniform radiation, located between radiowaves and infrared light, was accidental. Known today as Cosmic Microwave background (CMB), this diffuse radiation is commonly interpreted as a fossil light released in an early hot and dense universe and constitutes today the main 'pilar' of the big bang cosmology. Considerable efforts have been devoted to derive fundamental cosmological parameters from the characteristics of this radiation that led to a surprising universe that is shaped by at least three major unknown components: inflation, dark matter and dark energy. This is an important weakness of the present consensus cosmological model that justifies raising several questions on the CMB interpretation. Can we consider its cosmological nature as undisputable? Do other possible interpretations exist in the context of other cosmological theories or…
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Taxonomy
TopicsCosmology and Gravitation Theories · Space Science and Extraterrestrial Life · Relativity and Gravitational Theory
