학술논문

Neutrinos and Cosmic Rays Observed by IceCube
Document Type
Working Paper
Author
IceCube CollaborationAartsen, M. G.Ackermann, M.Adams, J.Aguilar, J. A.Ahlers, M.Ahrens, M.Samarai, I. AlAltmann, D.Andeen, K.Anderson, T.Ansseau, I.Anton, G.Archinger, M.Argüelles, C.Auffenberg, J.Axani, S.Bai, X.Barwick, S. W.Baum, V.Bay, R.Beatty, J. J.Tjus, J. BeckerBecker, K. -H.BenZvi, S.Berley, D.Bernardini, E.Bernhard, A.Besson, D. Z.Binder, G.Bindig, D.Blaufuss, E.Blot, S.Bohm, C.Börner, M.Bos, F.Bose, D.Böser, S.Botner, O.Braun, J.Brayeur, L.Bretz, H. -P.Bron, S.Burgman, A.Carver, T.Casier, M.Cheung, E.Chirkin, D.Christov, A.Clark, K.Classen, L.Coenders, S.Collin, G. H.Conrad, J. M.Cowen, D. F.Cross, R.Day, M.de André, J. P. A. M.De Clercq, C.Rosendo, E. del PinoDembinski, H.De Ridder, S.Desiati, P.de Vries, K. D.de Wasseige, G.de With, M.DeYoung, T.Díaz-Vélez, J. C.di Lorenzo, V.Dujmovic, H.Dumm, J. P.Dunkman, M.Eberhardt, B.Ehrhardt, T.Eichmann, B.Eller, P.Euler, S.Evenson, P. A.Fahey, S.Fazely, A. R.Feintzeig, J.Felde, J.Filimonov, K.Finley, C.Flis, S.Fösig, C. -C.Franckowiak, A.Friedman, E.Fuchs, T.Gaisser, T. K.Gallagher, J.Gerhardt, L.Ghorbani, K.Giang, W.Gladstone, L.Glauch, T.Glüsenkamp, T.Goldschmidt, A.Gonzalez, J. G.Grant, D.Griffith, Z.Haack, C.Hallgren, A.Halzen, F.Hansen, E.Hansmann, T.Hanson, K.Hebecker, D.Heereman, D.Helbing, K.Hellauer, R.Hickford, S.Hignight, J.Hill, G. C.Hoffman, K. D.Hoffmann, R.Hoshina, K.Huang, F.Huber, M.Hultqvist, K.In, S.Ishihara, A.Jacobi, E.Japaridze, G. S.Jeong, M.Jero, K.Jones, B. J. P.Kang, W.Kappes, A.Karg, T.Karle, A.Katz, U.Kauer, M.Keivani, A.Kelley, J. L.Kheirandish, A.Kim, J.Kim, M.Kintscher, T.Kiryluk, J.Kittler, T.Klein, S. R.Kohnen, G.Koirala, R.Kolanoski, H.Konietz, R.Köpke, L.Kopper, C.Kopper, S.Koskinen, D. J.Kowalski, M.Krings, K.Kroll, M.Krückl, G.Krüger, C.Kunnen, J.Kunwar, S.Kurahashi, N.Kuwabara, T.Labare, M.Lanfranchi, J. L.Larson, M. J.Lauber, F.Lennarz, D.Lesiak-Bzdak, M.Leuermann, M.Lu, L.Lünemann, J.Madsen, J.Maggi, G.Mahn, K. B. M.Mancina, S.Mandelartz, M.Maruyama, R.Mase, K.Maunu, R.McNally, F.Meagher, K.Medici, M.Meier, M.Menne, T.Merino, G.Meures, T.Miarecki, S.Montaruli, T.Moulai, M.Nahnhauer, R.Naumann, U.Neer, G.Niederhausen, H.Nowicki, S. C.Nygren, D. R.Pollmann, A. ObertackeOlivas, A.O'Murchadha, A.Palczewski, T.Pandya, H.Pankova, D. V.Peiffer, P.Penek, Ö.Pepper, J. A.Heros, C. Pérez de losPieloth, D.Pinat, E.Price, P. B.Przybylski, G. T.Quinnan, M.Raab, C.Rädel, L.Rameez, M.Rawlins, K.Reimann, R.Relethford, B.Relich, M.Resconi, E.Rhode, W.Richman, M.Riedel, B.Robertson, S.Rongen, M.Rott, C.Ruhe, T.Ryckbosch, D.Rysewyk, D.Sabbatini, L.Herrera, S. E. SanchezSandrock, A.Sandroos, J.Sarkar, S.Satalecka, K.Schlunder, P.Schmidt, T.Schoenen, S.Schöneberg, S.Schumacher, L.Seckel, D.Seunarine, S.Soldin, D.Song, M.Spiczak, G. M.Spiering, C.Stachurska, J.Stanev, T.Stasik, A.Stettner, J.Steuer, A.Stezelberger, T.Stokstad, R. G.Stößl, A.Ström, R.Strotjohann, N. L.Sullivan, G. W.Sutherland, M.Taavola, H.Taboada, I.Tatar, J.Tenholt, F.Ter-Antonyan, S.Terliuk, A.Tešić, G.Tilav, S.Toale, P. A.Tobin, M. N.Toscano, S.Tosi, D.Tselengidou, M.Tung, C. F.Turcati, A.Unger, E.Usner, M.Vandenbroucke, J.van Eijndhoven, N.Vanheule, S.van Rossem, M.van Santen, J.Vehring, M.Voge, M.Vogel, E.Vraeghe, M.Walck, C.Wallace, A.Wallraff, M.Wandkowsky, N.Waza, A.Weaver, Ch.Weiss, M. J.Wendt, C.Westerhoff, S.Whelan, B. J.Wickmann, S.Wiebe, K.Wiebusch, C. H.Wille, L.Williams, D. R.Wills, L.Wolf, M.Wood, T. R.Woolsey, E.Woschnagg, K.Xu, D. L.Xu, X. W.Xu, Y.Yanez, J. P.Yodh, G.Yoshida, S.Zoll, M.
Source
Advances in Space Research 62 (2018) 2902-2930
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
The core mission of the IceCube Neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux, and constrains its origin. In addition, the spectrum, composition and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of IceCube data, and their implications on our understanding of cosmic rays.
Comment: Review article, to appear in Advances in Space Research, special issue "Origins of Cosmic Rays"