Abstract
Abstract
We propose a one-parametric extension of the Starobinsky R + R
2 model by adding the
R
+
m
2
β
2
3
/
2
term. The parameter m is the inflaton mass, which is determined in the same way as in the Starobinsky model, and β is a dimensionless constant. Using the Einstein frame and the scalar field potential, we get the inflationary parameters of the model proposed. The value of the tensor-to-scalar ratio r can be significantly larger than in the Starobinsky model. The considered inflationary model is in a good agreement with the current observational data. The corresponding scalar field potential is a polynomial of the exponential function.
Funder
Russian Foundation for Basic Research
Subject
Condensed Matter Physics,Mathematical Physics,Atomic and Molecular Physics, and Optics
Cited by
2 articles.
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