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 to our understanding of cosmic rays.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 2902-2930 |
| Number of pages | 29 |
| Journal | Advances in Space Research |
| Volume | 62 |
| Issue number | 10 |
| DOIs | |
| State | Published - Nov 15 2018 |
All Science Journal Classification (ASJC) codes
- Aerospace Engineering
- Astronomy and Astrophysics
- Geophysics
- Atmospheric Science
- Space and Planetary Science
- Earth and Planetary Sciences(all)
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Astrophysical neutrinos and cosmic rays observed by IceCube. / Aartsen, M. G.; Ackermann, M.; Adams, J. et al.
In: Advances in Space Research, Vol. 62, No. 10, 15.11.2018, p. 2902-2930.Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - Astrophysical neutrinos and cosmic rays observed by IceCube
AU - Aartsen, M. G.
AU - Ackermann, M.
AU - Adams, J.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Ahrens, M.
AU - Altmann, D.
AU - Andeen, K.
AU - Anderson, T.
AU - Ansseau, I.
AU - Anton, G.
AU - Archinger, M.
AU - Argüelles, C.
AU - Auffenberg, J.
AU - Axani, S.
AU - Bai, X.
AU - Barwick, S. W.
AU - Baum, V.
AU - Bay, R.
AU - Beatty, J. J.
AU - Becker Tjus, J.
AU - Becker, K. H.
AU - BenZvi, S.
AU - Berley, D.
AU - Bernardini, E.
AU - Bernhard, A.
AU - Besson, D. Z.
AU - Binder, G.
AU - Bindig, D.
AU - Bissok, M.
AU - Blaufuss, E.
AU - Blot, S.
AU - Bohm, C.
AU - Börner, M.
AU - Bos, F.
AU - Bose, D.
AU - Böser, S.
AU - Botner, O.
AU - Braun, J.
AU - Brayeur, L.
AU - Bretz, H. P.
AU - Bron, S.
AU - Burgman, A.
AU - Carver, T.
AU - Casier, M.
AU - Cheung, E.
AU - Chirkin, D.
AU - Christov, A.
AU - Clark, K.
AU - Classen, L.
AU - Coenders, S.
AU - Collin, G. H.
AU - Conrad, J. M.
AU - Cowen, D. F.
AU - Cross, R.
AU - Day, M.
AU - de André, J. P.A.M.
AU - De Clercq, C.
AU - del Pino Rosendo, E.
AU - Dembinski, H.
AU - De Ridder, S.
AU - Desiati, P.
AU - de Vries, K. D.
AU - de Wasseige, G.
AU - de With, M.
AU - DeYoung, T.
AU - Díaz-Vélez, J. C.
AU - di Lorenzo, V.
AU - Dujmovic, H.
AU - Dumm, J. P.
AU - Dunkman, M.
AU - Eberhardt, B.
AU - Ehrhardt, T.
AU - Eichmann, B.
AU - Eller, P.
AU - Euler, S.
AU - Evenson, P. A.
AU - Fahey, S.
AU - Fazely, A. R.
AU - Feintzeig, J.
AU - Felde, J.
AU - Filimonov, K.
AU - Finley, C.
AU - Flis, S.
AU - Fösig, C. C.
AU - Franckowiak, A.
AU - Friedman, E.
AU - Fuchs, T.
AU - Gaisser, T. K.
AU - Gallagher, J.
AU - Gerhardt, L.
AU - Ghorbani, K.
AU - Giang, W.
AU - Gladstone, L.
AU - Glauch, T.
AU - Glüsenkamp, T.
AU - Goldschmidt, A.
AU - Gonzalez, J. G.
AU - Grant, D.
AU - Griffith, Z.
AU - Haack, C.
AU - Hallgren, A.
AU - Halzen, F.
AU - Hansen, E.
AU - Hansmann, T.
AU - Hanson, K.
AU - Hebecker, D.
AU - Heereman, D.
AU - Helbing, K.
AU - Hellauer, R.
AU - Hickford, S.
AU - Hignight, J.
AU - Hill, G. C.
AU - Hoffman, K. D.
AU - Hoffmann, R.
AU - Holzapfel, K.
AU - Hoshina, K.
AU - Huang, F.
AU - Huber, M.
AU - Hultqvist, K.
AU - In, S.
AU - Ishihara, A.
AU - Jacobi, E.
AU - Japaridze, G. S.
AU - Jeong, M.
AU - Jero, K.
AU - Jones, B. J.P.
AU - Jurkovic, M.
AU - Kang, W.
AU - Kappes, A.
AU - Karg, T.
AU - Karle, A.
AU - Katz, U.
AU - Kauer, M.
AU - Keivani, A.
AU - Kelley, J. L.
AU - Kheirandish, A.
AU - Kim, J.
AU - Kim, M.
AU - Kintscher, T.
AU - Kiryluk, J.
AU - Kittler, T.
AU - Klein, S. R.
AU - Kohnen, G.
AU - Koirala, R.
AU - Kolanoski, H.
AU - Konietz, R.
AU - Köpke, L.
AU - Kopper, C.
AU - Kopper, S.
AU - Koskinen, D. J.
AU - Kowalski, M.
AU - Krings, K.
AU - Kroll, M.
AU - Krückl, G.
AU - Krüger, C.
AU - Kunnen, J.
AU - Kunwar, S.
AU - Kurahashi, N.
AU - Kuwabara, T.
AU - Labare, M.
AU - Lanfranchi, J. L.
AU - Larson, M. J.
AU - Lauber, F.
AU - Lennarz, D.
AU - Lesiak-Bzdak, M.
AU - Leuermann, M.
AU - Lu, L.
AU - Lünemann, J.
AU - Madsen, J.
AU - Maggi, G.
AU - Mahn, K. B.M.
AU - Mancina, S.
AU - Mandelartz, M.
AU - Maruyama, R.
AU - Mase, K.
AU - Maunu, R.
AU - McNally, F.
AU - Meagher, K.
AU - Medici, M.
AU - Meier, M.
AU - Meli, A.
AU - Menne, T.
AU - Merino, G.
AU - Meures, T.
AU - Miarecki, S.
AU - Montaruli, T.
AU - Moulai, M.
AU - Nahnhauer, R.
AU - Naumann, U.
AU - Neer, G.
AU - Niederhausen, H.
AU - Nowicki, S. C.
AU - Nygren, D. R.
AU - Obertacke Pollmann, A.
AU - Olivas, A.
AU - O'Murchadha, A.
AU - Palczewski, T.
AU - Pandya, H.
AU - Pankova, D. V.
AU - Peiffer, P.
AU - Penek,
AU - Pepper, J. A.
AU - Pérez de los Heros, C.
AU - Pieloth, D.
AU - Pinat, E.
AU - Price, P. B.
AU - Przybylski, G. T.
AU - Quinnan, M.
AU - Raab, C.
AU - Rädel, L.
AU - Rameez, M.
AU - Rawlins, K.
AU - Reimann, R.
AU - Relethford, B.
AU - Relich, M.
AU - Resconi, E.
AU - Rhode, W.
AU - Richman, M.
AU - Riedel, B.
AU - Robertson, S.
AU - Rongen, M.
AU - Rott, C.
AU - Ruhe, T.
AU - Ryckbosch, D.
AU - Rysewyk, D.
AU - Sabbatini, L.
AU - Sanchez Herrera, S. E.
AU - Sandrock, A.
AU - Sandroos, J.
AU - Sarkar, S.
AU - Satalecka, K.
AU - Schlunder, P.
AU - Schmidt, T.
AU - Schoenen, S.
AU - Schöneberg, S.
AU - Schumacher, L.
AU - Seckel, D.
AU - Seunarine, S.
AU - Soldin, D.
AU - Song, M.
AU - Spiczak, G. M.
AU - Spiering, C.
AU - Stanev, T.
AU - Stasik, A.
AU - Stettner, J.
AU - Steuer, A.
AU - Stezelberger, T.
AU - Stokstad, R. G.
AU - Stößl, A.
AU - Ström, R.
AU - Strotjohann, N. L.
AU - Sullivan, G. W.
AU - Sutherland, M.
AU - Taavola, H.
AU - Taboada, I.
AU - Tatar, J.
AU - Tenholt, F.
AU - Ter-Antonyan, S.
AU - Terliuk, A.
AU - Tešić, G.
AU - Tilav, S.
AU - Toale, P. A.
AU - Tobin, M. N.
AU - Toscano, S.
AU - Tosi, D.
AU - Tselengidou, M.
AU - Turcati, A.
AU - Unger, E.
AU - Usner, M.
AU - Vandenbroucke, J.
AU - van Eijndhoven, N.
AU - Vanheule, S.
AU - van Rossem, M.
AU - van Santen, J.
AU - Veenkamp, J.
AU - Vehring, M.
AU - Voge, M.
AU - Vogel, E.
AU - Vraeghe, M.
AU - Walck, C.
AU - Wallace, A.
AU - Wallraff, M.
AU - Wandkowsky, N.
AU - Weaver, Ch
AU - Weiss, M. J.
AU - Wendt, C.
AU - Westerhoff, S.
AU - Whelan, B. J.
AU - Wickmann, S.
AU - Wiebe, K.
AU - Wiebusch, C. H.
AU - Wille, L.
AU - Williams, D. R.
AU - Wills, L.
AU - Wolf, M.
AU - Wood, T. R.
AU - Woolsey, E.
AU - Woschnagg, K.
AU - Xu, D. L.
AU - Xu, X. W.
AU - Xu, Y.
AU - Yanez, J. P.
AU - Yodh, G.
AU - Yoshida, S.
AU - Zoll, M.
N1 - Funding Information: We acknowledge the support from the following agencies: U.S. National Science Foundation - Office of Polar Programs, U.S. National Science Foundation - Physics Division, University of Wisconsin Alumni Research Foundation , the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin - Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy , and National Energy Research Scientific Computing Center , the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada , WestGrid and Compute/Calcul Canada ; Swedish Research Council , Swedish Polar Research Secretariat , Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden ; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme , Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom ; Marsden Fund, New Zealand ; Australian Research Council ; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Villum Fonden , Danish National Research Foundation (DNRF), Denmark Funding Information: We acknowledge the support from the following agencies: U.S. National Science Foundation - Office of Polar Programs, U.S. National Science Foundation - Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin - Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, New Zealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Villum Fonden, Danish National Research Foundation (DNRF), Denmark Publisher Copyright: © 2017 COSPAR
PY - 2018/11/15
Y1 - 2018/11/15
N2 - 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 to our understanding of cosmic rays.
AB - 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 to our understanding of cosmic rays.
UR - http://www.scopus.com/inward/record.url?scp=85020655645&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85020655645&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2017.05.030
DO - 10.1016/j.asr.2017.05.030
M3 - Article
AN - SCOPUS:85020655645
VL - 62
SP - 2902
EP - 2930
JO - Advances in Space Research
JF - Advances in Space Research
SN - 0273-1177
IS - 10
ER -