Geodesic
Cosmological inflation models in the~kinetic approximation
Teoretičeskaâ i matematičeskaâ fizika, Tome 191 (2017) no. 2, pp. 354-365

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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.
Mots-clés : inflation, cosmological perturbation.
Keywords: scalar field 
@article{TMF_2017_191_2_a15,
     author = {I. V. Fomin},
     title = {Cosmological inflation models in the~kinetic approximation},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {354--365},
     publisher = {mathdoc},
     volume = {191},
     number = {2},
     year = {2017},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_2017_191_2_a15/}
}
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I. V. Fomin. Cosmological inflation models in the~kinetic approximation. Teoretičeskaâ i matematičeskaâ fizika, Tome 191 (2017) no. 2, pp. 354-365. http://geodesic.mathdoc.fr/item/TMF_2017_191_2_a15/