Model of Decaying Dark Energy Based on the Kaluza–Klein Theory


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On the basis of a scalar potential associated with Beltrami’s geometry – manifolds of constant negative curvature, the Klein–Gordon problem has been solved, making it possible, under the assumption of a physical structure of the fifth dimension (presumably a rich form of matter), to model on the basis of the Kaluza–Klein theory the hypothesis of decaying dark energy configuring the rates of expansion of the Universe.

Sobre autores

U. Zakirov

Institute of Physics of Kazan (Volga region) Federal University

Autor responsável pela correspondência
Email: zakirural@mail.ru
Rússia, Kazan’

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