Registration and software installation support Room: 503/1-001 - Council Chamber

Welcome Room: 503/1-001 - Council Chamber

Cosmic Rays I

• Pasquale Blasi (Gran Sasso Science Institute)

Room: 503/1-001 - Council Chamber Galactic energies, Acceleration, Propagation, gamma rays, spalation, etc.

Air Showers I

• Paolo Lipari (Universita e INFN, Roma I (IT))

Room: 503/1-001 - Council Chamber Heitler, Mathews, Cascade theory and approximations

Gamma observations with imaging Cherenkov Telescopes

• Abelardo Moralejo (Institut de Física d'Altes Energies)

Room: 503/1-001 - Council Chamber

Hands-On Session I

• Tanguy Pierog (KIT)
• Ralf Matthias Ulrich (KIT - Karlsruhe Institute of Technology (DE))

Room: 503/1-001 - Council Chamber Focus on CORSIKA

Inclusive Fluxes

• Anatoli Fedynitch

Room: 503/1-001 - Council Chamber Theory of cascades and inclusive fluxes, Numerical tools, physics of lepton fluxes

Radio emission

• Tim Huege (KIT)

Room: 503/1-001 - Council Chamber

Hands-on session II

• Felix Riehn (LIP Lisbon)

Room: 503/1-001 - Council Chamber Focus on CRMC

Dinner Chalet Suisse + Cave Valaisanne, Geneva

Cosmic Rays II

• Etienne Parizot (Université Paris Diderot / APC)

Room: 503/1-001 - Council Chamber Extragalactic and transition

ALICE

• Francesca Bellini (CERN)

Room: 503/1-001 - Council Chamber Results from ALICE

Hands-on session III

• Anatoli Fedynitch

Room: 503/1-001 - Council Chamber Focus on MCEq

Air Showers II

• Lorenzo Cazon (LIP)

Room: 503/1-001 - Council Chamber Air shower physics at UHECR, Muon production, p-air cross section, etc.

Towards EeV Astronomy: catching the sources of ultra-high-energy cosmic rays

• Kumiko Kotera (Institut d'Astrophysique de Paris)

Room: 500/1-001 - Main Auditorium The violent Universe still defies us, as the sources of ultra-high-energy cosmic rays remain unknown. Yet we have drastically increased the amount of information at very high energies in the last 5 years, with combined observations of cosmic rays, gamma rays, neutrinos, and gravitational waves. We will identify in this talk the multi-messenger data that can be relevant to solve this long-standing mystery, and compare them with the signatures predicted for the most promising source scenarios. For this purpose, we will recall the fate of primary cosmic rays in the source environment and in the intergalactic backgrounds during their flight to the Earth, and estimate their associated astroparticle emissions. We will give theoretical grounds and experimental prospects for successfully launching EeV Astronomy in the next decades. This would likely happen with the collection of hundreds of ultra-high-energy neutrinos, thanks to global multi-messenger networks and with ambitious high-sensitivity high-resolution experiments such as GRAND.