Exact and Approximate Solutions in the Friedmann Cosmology


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Abstract

A method for generating exact solutions of the equations of the scalar field dynamics in the case of flat Friedmann–Robertson–Walker space on the basis of form-invariant transformations is considered. A method for estimating the divergence of the exact and approximate solutions from the number of e-folds and the parameters of the cosmological perturbations is proposed.

About the authors

I. V. Fomin

Bauman Moscow State Technical University

Author for correspondence.
Email: ingvor@inbox.ru
Russian Federation, Moscow

S. V. Chervon

Ulyanovsk State Pedagogical University; Kwazulu-Natal University

Email: ingvor@inbox.ru
Russian Federation, Ul’yanovsk; Durban

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