Cosmological inflation models in the kinetic approximation


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Abstract

We consider the construction of cosmological inflation models with an approximate linear dependence of the kinetic energy of the scalar field on the state parameter. We compare the obtained solutions with known cosmological models and calculate the main parameters of cosmological perturbations.

About the authors

I. V. Fomin

Bauman Moscow State Technical University

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Email: ingvor@inbox.ru
Russian Federation, Moscow

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