High redshift constraints on dark energy models from the $E_{\mathrm{p},\mathrm{i}}$ -- $E_{\mathrm{iso}}$ correlation in GRBs

Marek Demianski, Ester Piedipalumbo, Disha Sawant +1

Here we test different models of dark energy beyond the standard cosmological constant scenario. We start considering the CPL parameterization of the equation of state (EOS), then…