Systematic parameter space study for the UHECR origin from GRBs in models with multiple internal shocks
Jonas Heinze, Daniel Biehl, Anatoli Fedynitch, Denise Boncioli, Annika, Rudolph, Walter Winter

TL;DR
This study systematically explores whether long-duration Gamma-Ray Bursts with multiple internal shocks can account for ultra-high energy cosmic rays, analyzing spectrum, composition, and neutrino fluxes under various model assumptions.
Contribution
It introduces a comprehensive model for GRBs with multiple internal shocks, assessing their viability as UHECR sources and predicting neutrino fluxes within observational constraints.
Findings
GRBs can explain UHECRs under various model assumptions.
Predicted neutrino fluxes are below current detection but accessible to future experiments.
Heavy mass fraction at injection exceeds 70% (95% CL).
Abstract
We scrutinize the paradigm that conventional long-duration Gamma-Ray Bursts (GRBs) are the dominant source of the ultra-high energy cosmic rays (UHECRs) within the internal shock scenario by describing UHECR spectrum and composition and by studying the predicted (source and cosmogenic) neutrino fluxes. Since it has been demonstrated that the stacking searches for astrophysical GRB neutrinos strongly constrain the parameter space in single-zone models, we focus on the dynamics of multiple collisions for which different messengers are expected to come from different regions of the same object. We propose a model which can describe both stochastic and deterministic engines, which we study in a systematic way. We find that GRBs can indeed describe the UHECRs for a wide range of different model assumptions with comparable quality albeit with the previously known problematic energy…
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