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This article is cited in 1 scientific paper (total in 1 paper)
Cosmological inflation models in the kinetic approximation
I. V. Fomin Bauman Moscow State Technical University, Moscow, Russia
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.
Keywords:
inflation, scalar field, cosmological perturbation.
Received: 26.02.2016 Revised: 14.03.2016
Citation:
I. V. Fomin, “Cosmological inflation models in the kinetic approximation”, TMF, 191:2 (2017), 354–365; Theoret. and Math. Phys., 191:2 (2017), 781–791
Linking options:
https://www.mathnet.ru/eng/tmf9177https://doi.org/10.4213/tmf9177 https://www.mathnet.ru/eng/tmf/v191/i2/p354
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Abstract page: | 350 | Full-text PDF : | 148 | References: | 41 | First page: | 16 |
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