New Constraints on all flavour Galactic diffuse neutrino emission with the ANTARES telescope
- Albert, A.
- André, M.
- Anghinolfi, M.
- Anton, G.
- Ardid, M.
- Aubert, J. J.
- Avgitas, T.
- Baret, B.
- Barrios Martí, J.
- Basa, S.
- Belhorma, B.
- Bertin, V.
- Biagi, S.
- Bormuth, R.
- Bourret, S.
- Bouwhuis, M. C.
- Bruijn, R.
- Brunner, J.
- Busto, J.
- CAPONE, Antonio
- Caramete, L.
- Carr, J.
- CELLI, SILVIA
- Cherkaoui El Moursli, R.
- Chiarusi, T.
- Circella, M.
- Coelho, J. A. B.
- Coleiro, A.
- Coniglione, R.
- Costantini, H.
- Coyle, P.
- Creusot, A.
- Díaz, A. F.
- Deschamps, A.
- DE BONIS, Giulia
- Distefano, C.
- DI PALMA, IRENE
- Domi, A.
- Donzaud, C.
- Dornic, D.
- Drouhin, D.
- Eberl, T.
- El Bojaddaini, I.
- El Khayati, N.
- Elsässer, D.
- Enzenhöfer, A.
- Ettahiri, A.
- Fassi, F.
- Felis, I.
- Fusco, L. A.
- Galatà, S.
- Gay, P.
- Giordano, V.
- Glotin, H.
- Grégoire, T.
- Gracia Ruiz, R.
- Graf, K.
- Hallmann, S.
- van Haren, H.
- Heijboer, A. J.
- Hello, Y.
- Hernández Rey, J. J.
- Hößl, J.
- Hofestädt, J.
- Hugon, C.
- Illuminati, G.
- James, C. W.
- de Jong, M.
- Jongen, M.
- Kadler, M.
- Kalekin, O.
- Katz, U.
- Kießling, D.
- Kouchner, A.
- Kreter, M.
- Kreykenbohm, I.
- Kulikovskiy, V.
- Lachaud, C.
- Lahmann, R.
- Lefèvre, D.
- Leonora, E.
- Lotze, M.
- Loucatos, S.
- Marcelin, M.
- Margiotta, A.
- Marinelli, A.
- Martínez Mora, J. A.
- Mele, R.
- Melis, K.
- Michael, T.
- Migliozzi, P.
- Moussa, A.
- Navas, S.
- Nezri, E.
- Organokov, M.
- Păvălaş, G. E.
- Pellegrino, C.
- PERRINA, CHIARA
- Piattelli, P.
- Popa, V.
- Pradier, T.
- Quinn, L.
- Racca, C.
- Riccobene, G.
- Sánchez Losa, A.
- Saldaña, M.
- Salvadori, I.
- Samtleben, D. F. E.
- Sanguineti, M.
- Sapienza, P.
- Schüssler, F.
- Sieger, C.
- Spurio, M.
- Stolarczyk, T.h.
- Taiuti, M.
- Tayalati, Y.
- Trovato, A.
- Turpin, D.
- Tönnis, C.
- Vallage, B.
- Van Elewyck, V.
- Versari, F.
- Vivolo, D.
- Vizzoca, A.
- Wilms, J.
- Zornoza, J. D.
- Zúñiga, J.
- Gaggero, D.
- Grasso, D.
DOIAbstract
The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization of this flux will shed light on Galactic accelerator features, gas distribution morphology and Galactic cosmic ray transport. The central Galactic plane can be the site of an enhanced neutrino production, thus leading to anisotropies in the extraterrestrial neutrino signal as measured by the IceCube Collaboration. The ANTARES neutrino telescope, located in the Mediterranean Sea, offers a favourable view on this part of the sky, thereby allowing for a contribution to the determination of this flux. The expected diffuse Galactic neutrino emission can be obtained li...
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