Numerical analysis of the generalized Starobinsky inflationary model.

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 A S , n S and r for several values of p ≃ 1. We have found that the value of p = 1. 0 0 0 4 reproduces the value of A S , n S and r is in agreement with the current observational data. [ABSTRACT FROM AUTHOR]