Testing f (R) gravity models with quasar x-ray and UV fluxes

Abstract

Recently, active galactic nuclei (AGN) have been proposed as "standardizable candles,"thanks to an observed nonlinear relation between their x-ray and optical-ultraviolet (UV) luminosities, which provides an independent measurement of their distances. In this paper, we use these observables for the first time to estimate the parameters of f(R) gravity models (specifically, the Hu-Sawicki and the exponential models) together with the cosmological parameters. The importance of these types of modified gravity theories lies in the fact that they can explain the late time accelerated expansion of the universe without the inclusion of a dark energy component. We have also included other observable data to the analyses such as estimates of the Hubble parameter H(z) from cosmic chronometers (CCs), the Pantheon Type Ia (SnIa) supernovae compilation, and baryon acoustic oscillation (BAO) measurements. The 1σ inferred constraints using all datasets are b≤0.276, ωm=0.304-0.011+0.010, and H0=67.553-0.936+1.242 for the Hu-Sawicki model, and b=0.785-0.606+0.409 ωm=0.305-0.010+0.011 and H0=68.348-0.760+0.959 for the exponential one, but we stress that for both f(R) models results within 2σ are consistent with the Λ cold dark matter (CDM) model. Our results show that the allowed space parameter is restricted when both AGN and BAO data are added to CC and SnIa data, with the BAO dataset being the most restrictive one. We can conclude that both the ΛCDM model and small deviations from general relativity given by the f(R) models studied in this paper are allowed by the considered observational datasets.