First observation of PeV-energy neutrinos with IceCube

We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutr...

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Veröffentlicht in:Physical review letters 2013-07, Vol.111 (2), p.021103-021103, Article 021103
Hauptverfasser: Aartsen, M G, Abbasi, R, Abdou, Y, Ackermann, M, Adams, J, Aguilar, J A, Ahlers, M, Altmann, D, Auffenberg, J, Bai, X, Baker, M, Barwick, S W, Baum, V, Bay, R, Beatty, J J, Bechet, S, Becker Tjus, J, Becker, K-H, Bell, M, Benabderrahmane, M L, BenZvi, S, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Bertrand, D, Besson, D Z, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, D J, Bohaichuk, S, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, A M, Bruijn, R, Brunner, J, Carson, M, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Clevermann, F, Coenders, S, Cohen, S, Cowen, D F, Cruz Silva, A H, Danninger, M, Daughhetee, J, Davis, J C, De Clercq, C, De Ridder, S, Desiati, P, de With, M, DeYoung, T, Díaz-Vélez, J C, Dunkman, M, Eagan, R, Eberhardt, B, Eisch, J, Ellsworth, R W, Euler, S, Evenson, P A, Fadiran, O, Fazely, A R, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Franke, R, Frantzen, K, Fuchs, T, Gaisser, T K, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, J G, Goodman, J A, Góra, D, Grant, D, Groß, A, Gurtner, M, Ha, C, Haj Ismail, A
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Sprache:eng
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Zusammenfassung:We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutral-current ν(e,μ,τ) (ν(e,μ,τ)) or charged-current ν(e) (ν(e)) interactions within the IceCube detector. The events were discovered in a search for ultrahigh energy neutrinos using data corresponding to 615.9 days effective live time. The expected number of atmospheric background is 0.082±0.004(stat)(-0.057)(+0.041)(syst). The probability of observing two or more candidate events under the atmospheric background-only hypothesis is 2.9×10(-3) (2.8σ) taking into account the uncertainty on the expected number of background events. These two events could be a first indication of an astrophysical neutrino flux; the moderate significance, however, does not permit a definitive conclusion at this time.
ISSN:0031-9007
1079-7114
1079-7114
DOI:10.1103/physrevlett.111.021103