Measurement of the Atmospheric nu(e) Spectrum with IceCubeVisa övriga samt affilieringar
Ansvarig organisation
2015 (Engelska)Ingår i: Physical Review D, ISSN 1550-7998, E-ISSN 1550-2368, Vol. 91, nr 12Artikel i tidskrift (Refereegranskat) Published
Abstract [en]
We present a measurement of the atmospheric nu(e) spectrum at energies between 0.1 and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric nu(e) originate mainly from the decays of kaons produced in cosmic-ray air showers. This analysis selects 1078 fully contained events in 332 days of live time, and then identifies those consistent with particle showers. A likelihood analysis with improved event selection extends our previous measurement of the conventional v(e) fluxes to higher energies. The data constrain the conventional nu(e) flux to be 1.3(-0.3)(+0.4) times a baseline prediction from a Honda’s calculation, including the knee of the cosmic-ray spectrum. A fit to the kaon contribution (xi) to the neutrino flux finds a kaon component that is xi = 1.3(-0.4)(+0.5) times the baseline value. The fitted/measured prompt neutrino flux from charmed hadron decays strongly depends on the assumed astrophysical flux and shape. If the astrophysical component follows a power law, the result for the prompt flux is 0.0(-0.0)(+3.0) times a calculated flux based on the work by Enberg, Reno, and Sarcevic.
Ort, förlag, år, upplaga, sidor
2015. Vol. 91, nr 12
Nyckelord [en]
energy-spectrum neutrino flux amanda digitization performance cascades detector design system ice Astronomy & Astrophysics Physics
Forskningsämne
SWEDARP, IceCube
Identifikatorer
URN: urn:nbn:se:polar:diva-2152DOI: 10.1103/PhysRevD.91.122004OAI: oai:DiVA.org:polar-2152DiVA, id: diva2:851700
Forskningsfinansiär
Polarforskningssekretariatet
Anmärkning
ISI Document Delivery No.: CL5UK Times Cited: 0 Cited Reference Count: 67 Aartsen, M. G. Ackermann, M. Adams, J. Aguilar, J. A. Ahlers, M. Ahrens, M. Altmann, D. Anderson, T. Archinger, M. Arguelles, C. Arlen, T. C. Auffenberg, J. Bai, X. Barwick, S. W. Baum, V. Bay, R. Beatty, J. J. Tjus, J. Becker Becker, K. -H. Beiser, E. BenZvi, S. Berghaus, P. Berley, D. Bernardini, E. Bernhard, A. Besson, D. Z. Binder, G. Bindig, D. Bissok, M. Blaufuss, E. Blumenthal, J. Boersma, D. J. Bohm, C. Boerner, M. Bos, F. Bose, D. Boeser, S. Botner, O. Braun, J. Brayeur, L. Bretz, H. -P. Brown, A. M. Buzinsky, N. Casey, J. Casier, M. Cheung, E. Chirkin, D. Christov, A. Christy, B. Clark, K. Classen, L. Coenders, S. Cowen, D. F. Silva, A. H. Cruz Daughhetee, J. Davis, J. C. Day, M. de Andre, J. P. A. M. De Clercq, C. Dembinski, H. De Ridder, S. Desiati, P. de Vries, K. D. de Wasseige, G. de With, M. DeYoung, T. Diaz-Velez, J. C. Dumm, J. P. Dunkman, M. Eagan, R. Eberhardt, B. Ehrhardt, T. Eichmann, T. Euler, S. Evenson, P. A. Fadiran, O. Fahey, S. Fazely, A. R. Fedynitch, A. Feintzeig, J. Felde, J. Filimonov, K. Finley, C. Fischer-Wasels, T. Flis, S. Fuchs, T. Glagla, M. Gaisser, T. K. Gaior, R. Gallagher, J. Gerhardt, L. Ghorbani, K. Gier, D. Gladstone, L. Gluesenkamp, T. Goldschmidt, A. Golup, G. Gonzalez, J. G. Goodman, J. A. Gora, D. Grant, D. Gretskov, P. Groh, J. C. Gross, A. Ha, C. Haack, C. Ismail, A. Haj Hallgren, A. Halzen, F. Hansmann, B. Hanson, K. Hebecker, D. Heereman, D. Helbing, K. Hellauer, R. Hellwig, D. Hickford, S. Hignight, J. Hill, G. C. Hoffman, K. D. Hoffmann, R. Homeier, A. Hoshina, K. Huang, F. Huber, M. Huelsnitz, W. Hulth, P. O. Hultqvist, K. In, S. Ishihara, A. Jacobi, E. Japaridze, G. S. Jero, K. Jurkovic, M. Kaminsky, B. Kappes, A. Karg, T. Karle, A. Kauer, M. Keivani, A. Kelley, J. L. Kemp, J. Kheirandish, A. Kiryluk, J. Klaes, J. Klein, S. R. Kohnen, G. Kolanoski, H. Konietz, R. Koob, A. Koepke, L. Kopper, C. Kopper, S. Koskinen, D. J. Kowalski, M. Krings, K. Kroll, G. Kroll, M. Kunnen, J. Kurahashi, N. Kuwabara, T. Labare, M. Lanfranchi, J. L. Larson, M. J. Lesiak-Bzdak, M. Leuermann, M. Leuner, J. Luenemann, J. Madsen, J. Maggi, G. Mahn, K. B. M. Maruyama, R. Mase, K. Matis, H. S. Maunu, R. McNally, F. Meagher, K. Medici, M. Meli, A. Menne, T. Merino, G. Meures, T. Miarecki, S. Middell, E. Middlemas, E. Miller, J. Mohrmann, L. Montaruli, T. Morse, R. Nahnhauer, R. Naumann, U. Niederhausen, H. Nowicki, S. C. Nygren, D. R. Obertacke, A. Olivas, A. Omairat, A. O’Murchadha, A. Palczewski, T. Paul, L. Pepper, J. A. Heros, C. Perez de los Pfendner, C. Pieloth, D. Pinat, E. Posselt, J. Price, P. B. Przybylski, G. T. Puetz, J. Quinnan, M. Raedel, L. Rameez, M. Rawlins, K. Redl, P. Reimann, R. Relich, M. Resconi, E. Rhode, W. Richman, M. Richter, S. Riedel, B. Robertson, S. Rongen, M. Rott, C. Ruhe, T. Ruzybayev, B. Ryckbosch, D. Saba, S. M. Sabbatini, L. Sander, H. -G. Sandrock, A. Sandroos, J. Sarkar, S. Schatto, K. Scheriau, F. Schimp, M. Schmidt, T. Schmitz, M. Schoenen, S. Schoeneberg, S. Schoenwald, A. Schukraft, A. Schulte, L. Schulz, O. Seckel, D. Sestayo, Y. Seunarine, S. Shanidze, R. Smith, M. W. E. Soldin, D. Spiczak, G. M. Spiering, C. Stahlberg, M. Stamatikos, M. Stanev, T. Stanisha, N. A. Stasik, A. Stezelberger, T. Stokstad, R. G. Stoessl, A. Strahler, E. A. Strom, R. Strotjohann, N. L. Sullivan, G. W. Sutherland, M. Taavola, H. Taboada, I. Ter-Antonyan, S. Terliuk, A. Tesic, G. Tilav, S. Toale, P. A. Tobin, M. N. Tosi, D. Tselengidou, M. Unger, E. Usner, M. Vallecorsa, S. van Eijndhoven, N. Vandenbroucke, J. van Santen, J. Vanheule, S. Vehring, M. Voge, M. Vraeghe, M. Walck, C. Wallraff, M. Wandkowsky, N. Weaver, Ch. Wendt, C. Westerhoff, S. Whelan, B. J. Whitehorn, N. Wichary, C. Wiebe, K. Wiebusch, C. H. Wille, L. Williams, D. R. Wissing, H. Wolf, M. Wood, T. R. Woschnagg, K. Xu, D. L. Xu, X. W. Xu, Y. Yanez, J. P. Yodh, G. Yoshida, S. Zarzhitsky, P. Zoll, M. Maruyama, Reina/A-1064-2013 Maruyama, Reina/0000-0003-2794-512X U.S. National Science Foundation-Office of Polar Programs; U.S. National Science Foundation-Physics Division; University of Wisconsin Alumni Research Foundation; Grid Laboratory of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin-Madison; Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy; National Energy Research Scientific Computing Center; 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); 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 program; 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); Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Danish National Research Foundation, Denmark (DNRF) 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 program, 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); Danish National Research Foundation, Denmark (DNRF). 0 Amer physical soc College pk 1550-2368
2015-09-072015-09-072017-12-04Bibliografiskt granskad