Testing exponential f(R) gravity with CMB, DESI-DR2, and supernova data

One of the most popular competitors to the CDM paradigm as an explanation for the late-time acceleration of the universe is the modification of general relativity (GR), with models such as f ( R ) gravity among the main motivations. In this study, we consider an exponential f ( R ) gravity model as a possible extensions of the GR. The extra scalar degrees of freedom and their effects on the cosmic expansion and structure formation are continuously considered in this scenario. By combining the PPS, BBN, CC, DESI-DR2, and CMB datasets, we imposed limitations on this model. We performed a detailed statistical analysis of the free model parameter b together with the standard cosmological parameters. Our analysis yields values of H 0 that are slightly lower than those obtained in ΛCDM, indicating no significant relaxation of the H 0 tension. In contrast, the model predicts systematically higher values of S 8 , leading to a moderate alleviation of the S 8 tension by up to ∼ 1.2 σ when late-time datasets are included. Overall, these results demonstrate that although the considered f ( R ) gravity model does not resolve all cosmological tensions simultaneously, it provides a consistent improvement in the description of large-scale structure formation.