Sep 1 – 5, 2025
CERN
Europe/Zurich timezone

Session

Neutrinos

Sep 1, 2025, 9:30 AM
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium

CERN

400
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Conveners

Neutrinos

  • Joachim Kopp (CERN)

Neutrinos

  • Joachim Kopp (CERN)

Neutrinos

  • Andrea Caputo (U. Rome La Sapienza)

Neutrinos

  • Andrea Caputo (U. Rome La Sapienza)

Presentation materials

There are no materials yet.

  1. Clara Murgui Galvez (CERN), Joachim Kopp (CERN), Maria Pestana Da Luz Pereira Ramos, Miguel Escudero Abenza (CERN), Valerie Domcke (CERN)
    9/1/25, 9:30 AM
    Talk
  2. Patrick Foldenauer (Instituto de Física Teórica UAM/CSIC Madrid)
    9/1/25, 9:45 AM
    Invited Talk
  3. Damiano Francesco Giuseppe Fiorillo (Niels Bohr Institute, University of Copenhagen)
    9/1/25, 10:15 AM
    Invited Talk
  4. Dwaipayan Mukherjee (Tata Institute of Fundamental Research)
    9/1/25, 11:30 AM
    Talk

    A dense neutrino gas can exhibit collective flavor oscillations, driven by neutrino–neutrino forward scattering, which profoundly affect flavor evolution in core-collapse supernovae and the early Universe. While numerous studies have shown that a zero crossing in the difference of flavor distributions ($g_{\Gamma}$) of neutrinos determines the existence and character of instabilities, a...

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  5. Pietro Ghedini
    9/1/25, 11:35 AM
    Talk

    We investigate the clustering of neutrinos on both galactic and extragalactic scales, with the aim of probing their standard and non-standard properties. We focus on potential signatures of neutrino–dark matter interactions, which could imprint detectable features on the local distribution of cosmological neutrinos. Our phenomenological approach aims to produce testable predictions for future...

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  6. Nicolas Grimbaum Yamamoto (Université Libre de Bruxelles)
    9/1/25, 11:40 AM
    Talk

    Among the few methods to probe the early Universe through the observation of primordial particles, one possibility remains relatively unexplored: the detection of high-energy neutrinos emitted shortly after the Big Bang, originating from the decay or annihilation of early-Universe relics.

    We present a general study of this scenario. First, we emphasise that such neutrinos could exhibit...

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  7. Dibya S. Chattopadhyay (Oklahoma State University)
    9/1/25, 11:45 AM
    Talk

    The KM3NeT collaboration recently reported the observation of KM3-230213A, a neutrino event with an energy of 220 PeV, $\mathcal{O}(10)$ times more energetic than the highest-energy neutrino in IceCube’s catalog. Despite its larger effective area and longer data-taking period, IceCube has not observed similar events, leading to a tension quantified between ~2$\sigma$ and 3.5$\sigma$, depending...

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  8. Giuliano Giacalone
    9/1/25, 11:50 AM
    Talk

    Reducing uncertainties in theoretical evaluations of the nuclear matrix elements (NME) is crucial for designing and interpreting experiments aimed at discovering neutrinoless double beta decay. In this work, we identify a new class of observables, distinct from those employed in low-energy nuclear structure applications, that are strongly correlated with the values of the NME: momentum...

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  9. Matteo Parriciatu (Università degli Studi Roma Tre)
    9/1/25, 11:55 AM
    Talk

    In the presence of a finite modular flavour symmetry, fermion mass hierarchies may be generated by a slight deviation of the modulus from a symmetric point. This small parameter governing charged-lepton mass hierarchies may also be responsible for the breaking of lepton number in a symmetry-protected low-scale seesaw. In this talk, I will illustrate the implementation and the phenomenological...

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  10. Georg Raffelt (MPI Physik, Munich)
    9/1/25, 2:00 PM
    Invited Talk
  11. Jason Holt
    9/1/25, 3:45 PM
    Invited Talk
  12. Javier Menendez (University of Barcelona)
    9/1/25, 4:15 PM
    Invited Talk
  13. Julien Froustey (University of California, Berkeley (USA))
    9/1/25, 4:45 PM
    Invited Talk
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