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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

Astrophysical sources and backgrounds

26 Sept 2017, 14:30
Napoli

Napoli

Congress Center, Aula Magna, Via Partenope 36, Napoli

Conveners

Astrophysical sources and backgrounds

  • Maurizio Paolillo (NA)

Presentation materials

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  1. 29. IceCube spectral anomaly
    Dr Francesco Vissani (Gssi)
    26/09/2017, 14:30
    Astrophysical sources and backgrounds
    Talk (20'+5')
  2. 6. Expectations for high energy diffuse galactic neutrinos for different cosmic ray distributions
    Francesco Lorenzo Villante (AQ)
    26/09/2017, 14:55
    Astrophysical sources and backgrounds
    Talk (20'+5')
    The interaction of cosmic rays with the gas contained in our Galaxy is a guaranteed source of diffuse high energy neutrinos. We provide expectations for this component by considering different assumptions for the cosmic ray distribution in the Galaxy which are intended to cover the large uncertainty in cosmic ray propagation models. We calculate the angular dependence of the diffuse galactic...
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  3. 12. Looking for sources of astrophysical neutrinos
    Dmitri SEMIKOZ (APC, Paris)
    26/09/2017, 15:20
    Astrophysical sources and backgrounds
    Talk (20'+5')
    In this talk I'll discuss significance of the galactic component observation in the 4 years IceCube data. Also I'll review theoretical models, which can explain observed data both with Galactic and extra-galactic sources of neutrinos. In particular, I'll present model which at the same time explain UHECR and astrophysical neutrinos.
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  4. 35. Minimal models for extragalactic cosmic rays and neutrinos
    Michael Kachelriess (NTNU)
    26/09/2017, 15:45
    Astrophysical sources and backgrounds
    Talk (20'+5')
    I review attempts to explain in a unified way the experimental data on ultrahigh energy neutrinos and cosmic rays, using a single source class and obeying data on CR composition and limits on the extragalactic diffuse gamma-ray background.
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