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Teoreticheskaya i Matematicheskaya Fizika, 2017, Volume 191, Number 2, Pages 354–365
DOI: https://doi.org/10.4213/tmf9177 (Mi tmf9177) 		 
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
Full-text PDF (445 kB) Citations (1)
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DOI: https://doi.org/10.4213/tmf9177
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.
Funding agency Grant number
Russian Foundation for Basic Research 16-02-00488_а
16-08-00618_а
This research is supported by the Russian Foundation for Basic Research (Grant Nos. 16-02-00488_a and 16-08-00618_a).
Received: 26.02.2016
Revised: 14.03.2016
English version:
Theoretical and Mathematical Physics, 2017, Volume 191, Issue 2, Pages 781–791
DOI: https://doi.org/10.1134/S0040577917050166
Bibliographic databases:
Document Type: Article
PACS: 04.20.-q, 04.25.-g
MSC: 83F05
Language: Russian
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
Citation in format AMSBIB
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  • https://www.mathnet.ru/eng/tmf/v191/i2/p354
    • This publication is cited in the following 1 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    		Теоретическая и математическая физика Theoretical and Mathematical Physics
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