Joint constraints on Galactic diffuse neutrino emission from ANTARES and IceCube
Creators: name: Albert, A.
name: André, M.
name: Anghinolfi, M.
name: Ardid, M.
name: Aubert, J. -J.
name: Aublin, J.
name: Avgitas, T.
name: Baret, B.
name: Barrios-Martí, J.
name: Basa, S.
name: Belhorma, B.
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name: Boumaaza, J.
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name: Bruijn, R.
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name: Chabab, M.
name: Moursli, R. Cherkaoui El
name: Chiarusi, T.
name: Circella, M.
name: Coelho, J. A. B.
name: Coleiro, A.
name: Colomer, M.
name: Coniglione, R.
name: Costantini, H.
name: Coyle, P.
name: Creusot, A.
name: Díaz, A. F.
name: Deschamps, A.
name: Distefano, C.
name: Di Palma, I.
name: Domi, A.
name: Donzaud, C.
name: Dornic, D.
name: Drouhin, D.
name: Eberl, T.
name: Bojaddaini, I. El
name: Khayati, N. El
name: Elsässer, D.
name: Enzenhöfer, A.
name: Ettahiri, A.
name: Fassi, F.
name: Felis, I.
name: Fermani, P.
name: Ferrara, G.
name: Fusco, L.
name: Gay, P.
name: Glotin, H.
name: Grégoire, T.
name: Ruiz, R. Gracia
name: Graf, K.
name: Hallmann, S.
name: van Haren, H.
name: Heijboer, A. J.
name: Hello, Y.
name: Hernández-Rey, J. J.
name: Hößl, J.
name: Hofestädt, J.
name: Illuminati, G.
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name: de Jong, M.
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Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: The existence of diffuse Galactic neutrino production is expected from cosmic ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offering the opportunity to test the products of Galactic cosmic ray interactions up to energies of hundreds of TeV. Here we present a search for this production using ten years of ANTARES track and shower data, as well as seven years of IceCube track data. The data are combined into a joint likelihood test for neutrino emission according to the KRA$_γ$ model assuming a 5 PeV per nucleon Galactic cosmic ray cutoff. No significant excess is found. As a consequence, the limits presented in this work start constraining the model parameter space for Galactic cosmic ray production and transport.
description: 5 figures