26–28 févr. 2020
Institut d’Astrophysique de Paris
Fuseau horaire Europe/Paris

High-energy neutrinos from cosmic ray interactions in the Local Bubble

28 févr. 2020, 15:15
15m
Amphithéatre (Institut d’Astrophysique de Paris)

Amphithéatre

Institut d’Astrophysique de Paris

Institut d’Astrophysique de Paris 98 bis, boulevard Arago 75014 Paris
Oral presentation Astrophysics Talk

Orateur

makarim bouyahiaoui

Description

We study the possibility that a local nearby supernova Vela is responsible for the knee in the cosmic rays spectrum. This source could also explain the excess of IceCube neutrinos with energies E > 100TeV and gamma-ray excess at high Galactic latitudes at energies E > 300 GeV in FermiLat data. Our work takes into account the presence of the Local Bubble which plays the role of a shield for cosmic rays flux and target to produce neutrinos and gamma rays from primordial Vela PeV protons.

Field InterStellar Medium

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