Numerical analysis of the generalized Starobinsky inflationary model
Abstract
In this work we study numerically one kind of generalization of the Starobinsky inflationary model (power-law type), which is characterized by the parameter p. In order to find the parameter p that fixes with observations, we compute the cosmological parameters AS, nS, and r for several values of p 1. We have found that the value of p=1.0004 reproduces the value of AS, n, and r in agreement with current observational data.
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