Cosmological constraints on $\gamma$-gravity models

TL;DR

This study tests the $\gamma$-gravity $f(R)$ model against recent cosmological data, finding it consistent with observations and statistically comparable to $\Lambda$CDM, offering a viable alternative for testing deviations from General Relativity.

Contribution

The paper provides the first comprehensive observational constraints on the $\gamma$-gravity $f(R)$ model using multiple cosmological datasets and compares its statistical performance with $\Lambda$CDM.

Findings

$\gamma$-gravity model fits current data well.

Statistically equivalent to $\Lambda$CDM according to AIC.

Higher best-fit $f(R)$ values may help address halo-mass function issues.

Abstract

In this paper we place observational constraints on the well-known $\gamma$-gravity $f(R)$ model using the latest cosmological data, namely we use the latest growth rate, Cosmic Microwave Background, Baryon Acoustic Oscillations, Supernovae type Ia and Hubble parameter data. Performing a joint likelihood analysis we find that the $\gamma$-gravity model is in very good agreement with observations. Utilizing the AIC statistical test we statistically compare the current $f(R)$ model with $\Lambda$CDM cosmology and find that they are statistically equivalent. Therefore, $\gamma$-gravity can be seen as a useful scenario toward testing deviations from General Relativity. Finally, we note that we find somewhat higher values for the $f(R)$ best-fit values compared to those mentioned in the past in the literature and we argue that this could potential alleviate the halo-mass function problem.