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Calculation of the precision parameters of relic radiation in the Starobinsky inflationary model S. K. Saburov

By: Saburov, S. KMaterial type: ArticleArticleContent type: Текст Media type: электронный Subject(s): модифицированная гравитация | реликтовое излучение | космическая инфляция | инфляционная модель ВселеннойGenre/Form: статьи в журналах Online resources: Click here to access online In: Russian physics journal Vol. 65, № 2. P. 250-259Abstract: The Starobinsky inflationary model of theoretical description of the early Universe is used to calculate the precision parameters of relic microwave radiation by analytical and numerical methods with allowance for subleading corrections to the number of e-foldings characterizing duration of inflation. The Mukhanov–Chibisov formula for the spectral index of scalar relic radiation perturbations is generalized with accuracy up to cubic terms of the number e-foldings.
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The Starobinsky inflationary model of theoretical description of the early Universe is used to calculate the precision parameters of relic microwave radiation by analytical and numerical methods with allowance for subleading corrections to the number of e-foldings characterizing duration of inflation. The Mukhanov–Chibisov formula for the spectral index of scalar relic radiation perturbations is generalized with accuracy up to cubic terms of the number e-foldings.

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