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.
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
This publication is cited in the following 1 articles:
I. Fomin, S. Chervon, “Exact and slow-roll solutions for exponential power-law inflation connected with modified gravity and observational constraints”, Universe, 6:11 (2020), 199