학술논문

Limits on the nuclearite flux using the ANTARES neutrino telescope
Document Type
Working Paper
Author
ANTARES CollaborationAlbert, A.Alves, S.André, M.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 ElChiarusi, T.Circella, M.Coelho, J. A. B.Coleiro, A.Coniglione, R.Coyle, P.Creusot, A.Díaz, A. F.de Wasseige, G.De Martino, B.Distefano, C.Di Palma, I.Domi, A.Donzaud, C.Dornic, D.Drouhin, D.Eberl, T.van Eeden, T.van Eijk, D.Khayati, N. ElEnzenhöfer, A.Fermani, P.Ferrara, G.Filippini, F.Fusco, L.García, J.Gay, P.Glotin, H.Gozzini, R.Ruiz, R. GraciaGraf, K.Guidi, C.Hallmann, S.van Haren, H.Heijboer, A. J.Hello, Y.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.Kouchner, A.Kreykenbohm, I.Kulikovskiy, V.Lahmann, R.Lamoureux, M.Breton, R. LeLefèvre, D.Leonora, E.Levi, G.Stum, S. LeLopez-Coto, D.Loucatos, S.Maderer, L.Manczak, J.Marcelin, M.Margiotta, A.Marinelli, A.Martínez-Mora, J. A.Melis, K.Migliozzi, P.Moussa, A.Muller, R.Nauta, L.Navas, S.Nezri, E.Fearraigh, B. ÓPăun, 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. SalesaSamtleben, 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.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
In this work, a search for nuclearites of strange quark matter by using nine years of ANTARES data taken in the period 2009-2017 is presented. The passage through matter of these particles is simulated %according to the model of de R\'{u}jula and Glashow taking into account a detailed description of the detector response to nuclearites and of the data acquisition conditions. A down-going flux of cosmic nuclearites with Galactic velocities ($\beta = 10^{-3}$) was considered for this study. The mass threshold for detecting these particles at the detector level is \mbox{ $4 \times 10^{13}$ GeV/c$^{2}$}. Upper limits on the nuclearite flux for masses up to $10^{17}$ GeV/c$^{2}$ at the level of $\sim 5 \times 10^{-17}$ cm$^{-2}$ s$^{-1}$ sr$^{-1}$ are obtained. These are the first upper limits on nuclearites established with a neutrino telescope and the most stringent ever set for Galactic velocities.
Comment: 17 pages, 7 figures