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Generalized Exact Solutions in the Friedmann Cosmology


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Abstract

Methods for obtaining exact solutions of the dynamical equations in Friedmann–Robertson–Walker spacetime for cosmological models with a scalar field and matter fields or nonzero curvature are considered on the basis of a representation of the main cosmological parameters as functions of the number of e-folds and direct substitution of the scale factor.

About the authors

I. V. Fomin

Bauman Moscow State Technical University (National Research University)

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Email: ingvor@inbox.ru
Russian Federation, Moscow

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