Testing hadronic and photohadronic interactions as responsible for ultrahigh energy cosmic rays and neutrino fluxes from starburst galaxies

A Condorelli, D Boncioli, E Peretti, S Petrera - Physical Review D, 2023 - APS
We test the hypothesis of starburst galaxies as sources of ultrahigh energy cosmic rays and
high energy neutrinos. The computation of interactions of ultrahigh energy cosmic rays in the …

Impact of Galaxy Clusters on the Propagation of Ultrahigh-energy Cosmic Rays

A Condorelli, J Biteau, R Adam - The Astrophysical Journal, 2023 - iopscience.iop.org
Galaxy clusters are the largest objects in the Universe kept together by gravity. Most of their
baryonic content is made of a magnetized diffuse plasma. We investigate the impact of such …

Joint measurement of the ultra-high-energy neutrino spectrum and cross section

VB Valera, M Bustamante, O Mena - arXiv preprint arXiv:2308.07709, 2023 - arxiv.org
Soon, a new generation of neutrino telescopes, presently under planning, will target the
discovery of ultra-high-energy (UHE) neutrinos of cosmic origin, with energies higher than …

[HTML][HTML] The role of supernovae inside AGN jets in UHECR acceleration

V Bosch-Ramon - Astronomy & Astrophysics, 2023 - aanda.org
Context. Jets of active galactic nuclei are potential accelerators of ultra high-energy cosmic
rays. Supernovae can occur inside these jets and contribute to cosmic ray acceleration …

[PDF][PDF] Studies of the mass composition of cosmic rays and proton-proton interaction cross-sections at ultra-high energies with the Pierre Auger Observatory

A Abdul Halim, H Abreu, M Aglietta, T Bister… - 2023 - repository.ubn.ru.nl
Knowledge of the primary composition of cosmic rays is very important for understanding the
nature and origin of ultra-high-energy cosmic rays (UHECR). As cosmic rays propagate …

[PDF][PDF] Ultra-high-energy cosmic rays from accretion shocks of galaxy clusters and filaments

P Simeon, N Globus, KSS Barrow… - Proceedings of 38th …, 2023 - inspirehep.net
The challenge of explaining the origin of ultra-high-energy cosmic rays (UHECRs) is the
need for a source class that can accelerate particles up to 100 EeV and that is abundant …

[PDF][PDF] Constraining models for the origin of ultra-high-energy cosmic rays with spectrum, composition, and arrival direction data measured at the Pierre Auger …

T Bister, A Abdul Halim, H Abreu, M Aglietta… - 2023 - repository.ubn.ru.nl
Ultra-high-energy cosmic rays (UHECRs) persist as an area of profound investigation, with
the quest to unveil their origin on the brink of realization. Recent findings indicate a potential …

Anisotropies, large and small

T Bister, G Farrar - arXiv preprint arXiv:2308.10678, 2023 - arxiv.org
We report on several new results using anisotropies of UHECRs. We improve and extend
the work of Ding, Globus and Farrar, who modeled the UHECR dipole assuming sources …

Highlights from the Pierre Auger Observatory

F Salamida - arXiv preprint arXiv:2312.14673, 2023 - arxiv.org
The Pierre Auger Observatory is a unique facility designed to study ultra-high energy cosmic
rays, with energies up to 10$^{20} $ eV and beyond. The Observatory is located in Argentina …

The Pierre Auger Observatory Open Data

AA Halim, P Abreu, M Aglietta, I Allekotte… - arXiv preprint arXiv …, 2023 - arxiv.org
The Pierre Auger Collaboration has embraced the concept of open access to their research
data since its foundation, with the aim of giving access to the widest possible community. A …