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 [Formula: see text]. In order to find the parameter [Formula: see text] that fixes with observations, we compute the cosmological parameters [Formula: see text], [Formula: see text] and [Formula: see text] for several values of [Formula: see text]. We have found that the value of [Formula: see text] reproduces the value of [Formula: see text], [Formula: see text] and [Formula: see text] is in agreement with the current observational data.
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