7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Prospects in dark energy cosmology through the calibrated Ep,I-Eiso correlation

9 Jul 2024, 15:00
30m
Tosti (Aurum)

Tosti

Aurum

Largo Gardone Riviera, Pescara, Italy
Invited talk in a parallel session Current Status of the H_0 and growth tensions: theoretical models and model-independent constraints Current status of the H_0 and growth tensions: theoretical models and model-independent constraints

Speaker

Prof. Ester Piedipalumbo (Department of Physics "E. Pancini", University of Naples Federico II)

Description

Using a new sample consisting of 264 GRBs with measured redshifts and spectra, we applied different techniques to calibrate the Ep,I-Eiso correlation against the type Ia SN data to build a calibrated GRB Hubble diagram. We tested the possible redshift dependence of the correlation and its effect on the Hubble diagram to investigate the tension with the flat ΛCDM model and the dark energy equation of state.

Primary authors

Prof. Ester Piedipalumbo (Department of Physics "E. Pancini", University of Naples Federico II) Prof. Marek Demianski (Institute for Theoretical Physics, University of Warsaw, Pasteura 5, PL-02-093 Warsaw, Poland; Department of Astronomy, Williams College, Williamstown, MA 01267, USA) Dr Lorenzo Amati (INAF-IASF, Sezione di Bologna, via Gobetti 101, I-40129 Bologna, Italy)

Presentation materials

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