TL;DR
This study investigates constraints on modified gravity parameters using various datasets, revealing a tension between Planck and lensing data with implications for testing General Relativity at cosmological scales.
Contribution
It introduces a one-parameter-at-a-time analysis of MG parameters, highlighting dataset tensions and the role of lensing in constraining modified gravity models.
Findings
Planck data shows a 3.9-$\sigma$ tension with GR for certain MG models.
Lensing data reduces or removes tensions with GR in MG constraints.
Two dataset groups exhibit a dichotomy, possibly due to systematics or modeling issues.
Abstract
An important route to testing General Relativity (GR) at cosmological scales is usually done by constraining modified gravity (MG) parameters added to the Einstein perturbed equations. Most studies have analyzed so far constraints on pairs of MG parameters, but here, we explore constraints on one parameter at a time while fixing the other at its GR value. This allows us to analyze various models while benefiting from a stronger constraining power from the data. We also explore which specific datasets are in tension with GR. We find that models with (, ) and (, ) exhibit a 3.9- and 3.8- departure from GR when using Planck18+SNe+BAO, while (, ) shows a tension of 3.4-. We find no tension with GR for models with the MG parameter fixed to its GR value. Using a Bayesian model selection analysis, we find that some…
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