UHECR from high- and low-luminosity GRBs


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  • <p>ICRC</p>


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  • uploaded June 25, 2021

Discussion timeslot (ZOOM-Meeting): 13. July 2021 - 12:00
ZOOM-Meeting URL: https://desy.zoom.us/j/92210078166
ZOOM-Meeting ID: 92210078166
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/02-Constraining-UHECR-sources-CRI/63
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

'We discuss the production of multiple messengers including UHECR, EM radiation and neutrinos in Gamma-Ray Bursts in models with multiple interaction regions.rnWe demonstrate that standard high-luminosity bursts can explain the UHECR spectrum as as measured by the Pierre Auger Observatory, and derive the required source injection composition for different engine realisations. We discuss how multi-messenger observations can be used to discriminate between models by explicitly calculating the expected source and cosmogenic neutrino fluxes as well as the photon light curves. In addition, a separate population of LL-GRBs may exist, for which we show that different nuclei can indeed reach UHECR energies. For this purpose, we self-consistently model the radiation fields in prototypes inspired by real GRBs. We connect the maximal energies attainable for cosmic-ray nuclei to a possible VHE and HE component in the SED.'

Authors: Daniel Biehl | Zeljka Bosnjak | Iftach Sadeh | Jonas Heinze | Walter Winter | Denise Boncioli | Annika Rudolph | Anatoli Fedynitch
Indico-ID: 404
Proceeding URL: https://pos.sissa.it/395/1000

Presenter: Annika Rudolph

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