Sep 23 – 27, 2024
Hotel Villa Tuscolana
Europe/Rome timezone

Session

IV Plenary

Sep 25, 2024, 11:20 AM
Aula Conferenze (Hotel Villa Tuscolana)

Aula Conferenze

Hotel Villa Tuscolana

Via del Tuscolo, km 1.5, 00044 Frascati RM

Conveners

IV Plenary

  • Antonio Capone (Istituto Nazionale di Fisica Nucleare)

Presentation materials

There are no materials yet.

  1. Giovanna Ferrara (Istituto Nazionale di Fisica Nucleare)
    9/25/24, 11:20 AM
    oral

    The ANTARES telescope was the first operational Neutrino Telescope in the Mediterranean Sea built at a depth of 2500 m offshore of Toulon, France, searching for astrophysical neutrinos in the TeV- PeV energy range. Debuting in May 2008, the ANTARES neutrino observatory served a 15-year mission until February 2022. Nestled deep in the Mediterranean Sea, its exceptional angular resolution made...

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  2. Rosa Coniglione (Istituto Nazionale di Fisica Nucleare)
    9/25/24, 11:45 AM
    oral

    The KM3NeT collaboration is building two underwater neutrino detectors in the Mediterranean: the ARCA (Astroparticle Research with Cosmics in the Abyss) and ORCA (Oscillation Research with Cosmics in the Abyss) detectors.
    ARCA is located off the Sicilian coast of Capo Passero and aims to detect and identify astrophysical neutrino sources. The ORCA detector, located off the French coast of...

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  3. Juan Antonio Aguilar Sánchez (Université Libre de Bruxelles)
    9/25/24, 12:10 PM
    oral

    Over the past decade, the IceCube Neutrino Observatory, situated at the geographical South Pole, has opened a new window to observe and study the high-energy Universe. In 2013, IceCube discovered the first high-energy neutrino events confirming the existence of a diffuse flux of astrophysical neutrinos. The level of this neutrino flux implies a much richer hadronic activity in the non-thermal...

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  4. Amy Connolly
    9/25/24, 12:35 PM
    oral

    Ultra-high energy (UHE) neutrinos are an important missing piece of the rapidly growing field of multi-messenger astrophysics. They carry information about the nature of the sources of the highest energy cosmic rays and may also provide hints of any new physics at O(100 TeV). There are many strategies being pursued to detect UHE neutrinos, and the most promising ones utilize signatures at...

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