Study of some cosmological parameters in logarithmic corrected f(R) gravitational model with swampland conjectures

Abstract

In this paper, we use corrected [Formula: see text] gravitational model which is a polynomial function with a logarithmic term. We employ the slow-roll conditions and obtain the number of cosmological parameters. This helps us to verify the swampland conjectures which guarantees validation of low energy quantum field theory. The obtained results show that the corresponding model is consistent with the swampland conjectures. Also, the upper and lower limits of the parameter [Formula: see text] are, respectively, 0.15 and 0.0033. Finally, by using scalar spectrum index [Formula: see text] and tensor-to-scalar ratio [Formula: see text] relations and comparing with the Planck 2018 data, we obtain the coefficients [Formula: see text], [Formula: see text] and [Formula: see text]. Also, the corresponding results are constructed by several figures, literature and also Planck 2018 data.