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Perspectives in Astroparticle physics from High Energy Neutrinos

25–26 Sept 2017
Napoli
Europe/Rome timezone

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Session

New physics at high-energy neutrino telescopes

26 Sept 2017, 11:20
Napoli

Napoli

Congress Center, Aula Magna, Via Partenope 36, Napoli

Conveners

New physics at high-energy neutrino telescopes

  • Pasquale Dario Serpico (CNRS, Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTh), France)

Presentation materials

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  1. 28. Probing origin of matter from RH neutrinos with IceCube
    Pasquale Di Bari (University of Southampton)
    26/09/2017, 11:20
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
  2. 7. A consistent model for leptogenesis, dark matter and the IceCube signal
    Dr Viviana Niro (ITP, Heidelberg)
    26/09/2017, 11:45
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
    We discuss a left-right symmetric extension of the Standard Model in which the three additional right-handed neutrinos play a central role in explaining the baryon asymmetry of the Universe, the dark matter abundance and the ultra energetic signal detected by the IceCube experiment. The energy spectrum and neutrino flux measured by IceCube are ascribed to the decays of the lightest...
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  3. 15. On the high-energy IceCube neutrinos
    Dr Sergio Palomares-Ruiz (IFIC (UV-CSIC))
    26/09/2017, 12:10
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
    The discovery of the high-energy neutrino flux by the IceCube detector has motivated a large number of studies in the literature to unravel their origin, from different scenarios within standard cosmic-ray sources to more exotic possibilities. In this talk, I will describe the evolution of the HESE data of IceCube and their main features and I will present the results of statistical analyses...
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  4. 36. Neutrino lines produced by DM annihilation: a model-building perspective for neutrino telescopes
    Prof. Thomas Hambye
    26/09/2017, 12:35
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
    In the near future, neutrino telescopes are expected to improve their sensitivity to the flux of monochromatic neutrinos produced by dark matter (DM) in our galaxy. This is illustrated by a new limit on the corresponding cross section that we derive from public IceCube data. In this context, we study which DM models could pro- duce an observable flux of monochromatic neutrinos from DM...
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