Published 2022 | Version v1
Journal article

Search for solar atmospheric neutrinos with the ANTARES neutrino telescope

Albert, A.
Alves, S.
André, M.
Anghinolfi, M.
Anton, G.
Ardid, M.
Ardid, S.
Aubert, J.-J.
Aublin, J.
Baret, B.
Basa, S.
Belhorma, B.
Bendahman, M.
Benfenati, F.
Bertin, V.
Biagi, S.
Bissinger, M.
Boumaaza, J.
Bouta, M.
Bouwhuis, M.C.
Brânzaş, H.
Bruijn, R.
Brunner, J.
Busto, J.
Caiffi, B.
Calvo, D.
Capone, A.
Caramete, L.
Carr, J.
Carretero, V.
Celli, S.
Chabab, M.
Chau, T.N.
Moursli, R. Cherkaoui El
Chiarusi, T.
Circella, M.
Coleiro, A.
Coniglione, R.
Coyle, P.
Creusot, A.
Díaz, A.F.
de Wasseige, G.
Distefano, C.
Di Palma, I.
Domi, A.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
van Eeden, T.
van Eijk, D.
Khayati, N. El
Enzenhöfer, A.
Fermani, P.
Ferrara, G.
Filippini, F.
Fusco, L.
Gatelet, Y.
Gay, P.
Glotin, H.
Gozzini, R.
Ruiz, R. Gracia
Graf, K.
Guidi, C.
Hallmann, S.
van Haren, H.
Heijboer, A.J.
Hello, Yann
Hernández-Rey, J.J.
Hössl, J.
Hofestädt, J.
Huang, F.
Illuminati, G.
James, C.W.
Jisse-Jung, B.
de Jong, M.
de Jong, P.
Kadler, M.
Kalekin, O.
Katz, U.
Khan-Chowdhury, N.R.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Breton, R. Le
Lestum, S.
Lefèvre, D.
Leonora, E.
Levi, G.
Lincetto, M.
Lopez-Coto, D.
Loucatos, S.
Maderer, L.
Manczak, J.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J.A.
Martino, B.
Melis, K.
Migliozzi, P.
Moussa, A.
Muller, R.
Nauta, L.
Navas, S.
Nezri, E.
Fearraigh, B.Ó.
Păun, A.
Păvălaş, G.E.
Pellegrino, C.
Perrin-Terrin, M.
Pestel, V.
Piattelli, P.
Pieterse, C.
Poirè, C.
Popa, V.
Pradier, T.
Randazzo, N.
Real, D.
Reck, S.
Riccobene, G.
Romanov, A.
Sánchez-Losa, A.
Greus, F. Salesa
Samtleben, D.F.E.
Sanguineti, M.
Sapienza, P.
Schnabel, J.
Schumann, J.
Schüssler, F.
Seneca, J.
Spurio, M.
Stolarczyk, Th.
Taiuti, M.
Tayalati, Y.
Tingay, S.J.
Vallage, B.
van Elewyck, V.
Versari, F.
Viola, S.
Vivolo, D.
Wilms, J.
Zavatarelli, S.
Zegarelli, A.
Zornoza, J.D.
Zúñiga, J.

Description

Solar Atmospheric Neutrinos (SAνs) are produced by the interaction of cosmic rays with the solar medium. The detection of SAνs would provide useful information on the composition of primary cosmic rays as well as the solar density. These neutrinos represent an irreducible source of background for indirect searches for dark matter towards the Sun and the measurement of their flux would allow for a better assessment of the uncertainties related to these searches. In this paper we report on the analysis performed, based on an unbinned likelihood maximisation, to search for SAνs with the ANTARES neutrino telescope. After analysing the data collected over 11 years, no evidence for a solar atmospheric neutrino signal has been found. An upper limit at 90% confidence level on the flux of solar atmospheric neutrinos has been obtained, equal to 7×10$^{-11}$ [ TeV$^{-1}$ cm$^{-2}$ s$^{-1}$] at E$_{ν}$ = 1 TeV for the reference cosmic ray model assumed.

Abstract

International audience

Additional details

Created:
February 22, 2023
Modified:
November 30, 2023