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Perspectives in Astroparticle physics from High Energy Neutrinos

Sep 25 – 26, 2017
Napoli
Europe/Rome timezone

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Session

Multimessenger physics & New physics at high-energy neutrino telescopes

Sep 25, 2017, 4:40 PM
Napoli

Napoli

Congress Center, Aula Magna, Via Partenope 36, Napoli

Conveners

Multimessenger physics & New physics at high-energy neutrino telescopes

  • Fabio Iocco (ICTP-SAIFR)

Presentation materials

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  1. 22. Future Wide Field of View Experiments: from Gamma-Ray Astronomy to Cosmic Rays
    Giuseppe Di Sciascio (ROMA2)
    9/25/17, 4:40 PM
    Multimessenger physics
    Talk (20'+5')
    The riddle of the origin of Cosmic Rays is unsolved since more than one century. The identification of the galactic sources able to accelerate particles beyond PeV energies is certainly one of the main open problems of high energy astrophysics. High energy gamma ray (and neutrino) observations are an essential probe of CRs, if gamma rays (and neutrinos) are produced by CRs interacting close to...
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  2. 23. UHECRs & Neutrinos
    Prof. Enrique Zas (IGFAE - University of Santiago)
    9/25/17, 5:05 PM
    Multimessenger physics
    Talk (20'+5')
  3. 3. High energy cosmic rays and the production of cosmogenic neutrinos and gamma-rays
    Roberto Aloisio (Gran Sasso Science Institute)
    9/25/17, 5:30 PM
    Multimessenger physics
    Talk (20'+5')
    We review the main features of ultra high energy cosmic rays propagation and the production of secondary cosmogenic particles such as neutrinos and gamma rays. We discuss the capabilities of the present and future observatories in the detection of these secondary particles, that has a paramount importance in constraining models for ultra high energy cosmic rays acceleration.
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  4. 24. PeV Neutrinos from Heavy Relic Decays in Early Universe
    Prof. Takeo Moroi
    9/25/17, 5:55 PM
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
  5. 5. Interpreting the IceCube neutrinos by decaying heavy DM
    Dr Arman Esmaili (Pontifícia Universidade Católica do Rio de Janeiro)
    9/25/17, 6:20 PM
    New physics at high-energy neutrino telescopes
    Talk (20'+5')
    I will discuss the possibility to interpret the IceCube data by PeV mass scale decaying Dark Matter. The generic signatures of this scenario, including its energy spectrum as well as the peculiar anisotropies will be discussed. Also possible future checks of this scenario by EAS experiments, both by detecting the prompt gamma ray flux from decaying dark matter, or the induced anisotropies in...
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