The models of cosmological inflation in the context of kinetic approximation

[摘要] In this work the building of models of cosmological inflation with approximate linear dependence of the scalar field kinetic energy on the state parameter is considered. The key parameters of cosmological perturbations are also calculated.

[发布机构] Physics Department, Bauman Moscow State Technical University, Moscow, Russia^1

[效力级别] 力学 [学科分类] 力学，机械学

[关键词] Approximate linear dependences;Cosmological perturbation;Scalar fields;State parameters