Averaging of the Equations of the Standard Cosmological Model over Rapid Oscillations


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Abstract

An averaging of the equations of the standard cosmological model (SCM) is carried out. It is shown that the main contribution to the macroscopic energy density of the scalar field comes from its microscopic oscillations with the Compton period. The effective macroscopic equation of state of the oscillations of the scalar field corresponds to the nonrelativistic limit.

About the authors

Yu. G. Ignat’ev

Lobachevsky Institute of Mathematics and Mechanics, Kazan’ Federal University

Author for correspondence.
Email: ignatev_yu@rambler.ru
Russian Federation, Kazan’

A. R. Samigullina

Lobachevsky Institute of Mathematics and Mechanics, Kazan’ Federal University

Email: ignatev_yu@rambler.ru
Russian Federation, Kazan’

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