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14th Cosmic-Ray International Studies and Multi-messenger Astroparticle Conference

12–17 Jul 2026
Sorrento
Europe/Rome timezone

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Session

Review

13 Jul 2026, 11:20
Itaca Hall (Sorrento)

Itaca Hall

Sorrento

Ulisse Deluxe Hostel Via del Mare, 22 - 80067 Sorrento – Napoli – Italy

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  1. 98. Hadronic Interactions and Cosmic-Ray Physics: A Comprehensive Review of the Muon Puzzle
    Dennis Soldin (University of Utah)
    13/07/2026, 11:20
    Review
    Oral

    High-energy cosmic rays interacting in the Earth’s atmosphere produce extensive air showers that are observed by large ground-based detector arrays. The properties of the primary cosmic ray must be inferred indirectly from the secondary particles measured at the surface, a process that relies strongly on theoretical models of hadronic interactions during shower development. Over the past two...

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  2. 36. Radio Detectors and their Applications in Astroparticle Physics
    Prof. Frank Schröder (Bartol Research Institute, Departement of Physics and Astronomy, University of Delaware)
    14/07/2026, 11:20
    Review
    Oral

    Radio detection of air showers has become a standard technique for indirect measurement of the highest energy Galactic and extragalactic cosmic rays. Geomagnetic and Askaryan radio emission are detectable around the clock, and a number of radio arrays have achieved measurement accuracies for the arrival direction, energy and position of the shower maximum competitive with traditional optical...

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  3. 31. Neutrino Astronomy: Current Status and Future Prospects
    Juan Antonio Aguilar Sánchez (Université Libre de Bruxelles)
    16/07/2026, 11:50
    Review
    Oral

    The detection of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory heralded the birth of neutrino astronomy, opening a new window onto the non-thermal Universe. Over the last years, IceCube has identified the first steady neutrino source emission, the Seyfert galaxy NGC 1068, as well as produced the first image of our own Milky Way captured with neutrinos. However, the...

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  4. 11. UHE gamma-ray sources: New insights into the most extreme particle accelerators in our Galaxy
    Gwenael Giacinti (APC Paris)
    17/07/2026, 11:20
    Review
    Oral

    The origin of very-high-energy Galactic cosmic-rays is currently hotly debated. Their most powerful sources in our Galaxy, also called “PeVatrons”, are expected to accelerate particles up to rigidities of at least a few PV, and possibly beyond. Such sources should also produce ultra-high-energy (UHE) gamma-rays. Recent observations by the LHAASO experiment with > 100 TeV gamma-rays show that...

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