Phys. Rev. D 76, 042008 (2007) [20 pages]
Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II
Abstract
References (50)
Citing Articles
A. Achterberg, 31 M. Ackermann, 33 J. Adams, 11 J. Ahrens, 21 K. Andeen, 20 J. Auffenberg, 32 X. Bai, 23 B. Baret, 9 S. W. Barwick, 16 R. Bay, 5 K. Beattie, 7 T. Becka, 21 J. K. Becker, 13 K.-H. Becker, 32 P. Berghaus, 8,15 D. Berley, 12 E. Bernardini, 33 D. Bertrand, 8 D. Z. Besson, 17 E. Blaufuss, 12 D. J. Boersma, 20 C. Bohm, 27 J. Bolmont, 33 S. Böser, 33 O. Botner, 30 A. Bouchta, 30 J. Braun, 20 T. Burgess, 27 T. Castermans, 22 D. Chirkin, 7 B. Christy, 12 J. Clem, 23 D. F. Cowen, 29,28 M. V. D'Agostino, 5 A. Davour, 30 C. T. Day, 7 C. De Clercq, 9 L. Demirörs, 23 F. Descamps, 14 P. Desiati, 20 T. DeYoung, 29 J. C. Diaz-Velez, 20 J. Dreyer, 13 J. P. Dumm, 20 M. R. Duvoort, 31 W. R. Edwards, 7 R. Ehrlich, 12 J. Eisch, 20 R. W. Ellsworth, 12 P. A. Evenson, 23 O. Fadiran, 3 A. R. Fazely, 4 K. Filimonov, 5 C. Finley, 20 M. M. Foerster, 29 B. D. Fox, 29 A. Franckowiak, 32 R. Franke, 33 T. K. Gaisser, 23 J. Gallagher, 19 R. Ganugapati, 20 H. Geenen, 32 L. Gerhardt, 16 A. Goldschmidt, 7 J. A. Goodman, 12 R. Gozzini, 21 T. Griesel, 21 A. Groß, 15 S. Grullon, 20 R. M. Gunasingha, 4 M. Gurtner, 32 C. Ha, 29 A. Hallgren, 30 F. Halzen, 20 K. Han, 11 K. Hanson, 20 D. Hardtke, 5 R. Hardtke, 26 J. E. Hart, 29 Y. Hasegawa, 10 T. Hauschildt, 23 D. Hays, 7 J. Heise, 31 K. Helbing, 32 M. Hellwig, 21 P. Herquet, 22 G. C. Hill, 20 J. Hodges, 20 K. D. Hoffman, 12 B. Hommez, 14 K. Hoshina, 20 D. Hubert, 9 B. Hughey, 20 J.-P. Hülß, 1 P. O. Hulth, 27 K. Hultqvist, 27 S. Hundertmark, 27 M. Inaba, 10 A. Ishihara, 10 J. Jacobsen, 7 G. S. Japaridze, 3 H. Johansson, 27 A. Jones, 7 J. M. Joseph, 7 K.-H. Kampert, 32 A. Kappes, 20 T. Karg, 32 A. Karle, 20 H. Kawai, 10 J. L. Kelley, 20 F. Kislat, 6 N. Kitamura, 20 S. R. Klein, 7 S. Klepser, 33 G. Kohnen, 22 H. Kolanoski, 6 L. Köpke, 21 M. Kowalski, 6 T. Kowarik, 21 M. Krasberg, 20 K. Kuehn, 16 M. Labare, 8 H. Landsman, 20 R. Lauer, 33 H. Leich, 33 D. Leier, 13 I. Liubarsky, 18 J. Lundberg, 30 J. Lünemann, 13 J. Madsen, 26 R. Maruyama, 20 K. Mase, 10 H. S. Matis, 7 T. McCauley, 7 C. P. McParland, 7 A. Meli, 13 T. Messarius, 13 P. Mészáros, 28,29 H. Miyamoto, 10 A. Mokhtarani, 7 T. Montaruli, 20 A. Morey, 5 R. Morse, 20 S. M. Movit, 28 K. Münich, 13 R. Nahnhauer, 33 J. W. Nam, 16 P. Nießen, 23 D. R. Nygren, 7 H. Ögelman, 20 A. Olivas, 12 S. Patton, 7 C. Peña-Garay, 25 C. Pérez de los Heros, 30 A. Piegsa, 21 D. Pieloth, 33 A. C. Pohl, 30 R. Porrata, 5 J. Pretz, 12 P. B. Price, 5 G. T. Przybylski, 7 K. Rawlins, 2 S. Razzaque, 28,29 E. Resconi, 15 W. Rhode, 13 M. Ribordy, 22 A. Rizzo, 9 S. Robbins, 32 P. Roth, 12 F. Rothmaier, 21 C. Rott, 29 D. Rutledge, 29 D. Ryckbosch, 14 H.-G. Sander, 21 S. Sarkar, 24 K. Satalecka, 33 S. Schlenstedt, 33 T. Schmidt, 12 D. Schneider, 20 D. Seckel, 23 B. Semburg, 32 S. H. Seo, 29 Y. Sestayo, 15 S. Seunarine, 11 A. Silvestri, 16 A. J. Smith, 12 M. Solarz, 5 C. Song, 20 J. E. Sopher, 7 G. M. Spiczak, 26 C. Spiering, 33 M. Stamatikos, 20 T. Stanev, 23 T. Stezelberger, 7 R. G. Stokstad, 7 M. C. Stoufer, 7 S. Stoyanov, 23 E. A. Strahler, 20 T. Straszheim, 12 K.-H. Sulanke, 33 G. W. Sullivan, 12 T. J. Sumner, 18 I. Taboada, 5 O. Tarasova, 33 A. Tepe, 32 L. Thollander, 27 S. Tilav, 23 M. Tluczykont, 33 P. A. Toale, 29 D. Tosi, 33 D. Turčan, 12 N. van Eijndhoven, 31 J. Vandenbroucke, 5 A. Van Overloop, 14 V. Viscomi, 29 B. Voigt, 33 W. Wagner, 29 C. Walck, 27 H. Waldmann, 33 M. Walter, 33 Y.-R. Wang, 20 C. Wendt, 20 C. H. Wiebusch, 1 C. Wiedemann, 27 G. Wikström, 27 D. R. Williams, 29 R. Wischnewski, 33 H. Wissing, 1 K. Woschnagg, 5 X. W. Xu, 4 G. Yodh, 16 S. Yoshida, 10 and J. D. Zornoza20
(IceCube Collaboration)
1III Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany
2Department of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Dr., Anchorage, Alaska 99508, USA
3CTSPS, Clark-Atlanta University, Atlanta, Georgia 30314, USA
4Department of Physics, Southern University, Baton Rouge, Louisiana 70813, USA
5Department of Physics, University of California, Berkeley, California 94720, USA
6Institut für Physik, Humboldt-Universität zu Berlin, D-12489 Berlin, Germany
7Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
8Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels, Belgium
9Vrije Universiteit Brussel, Dienst ELEM, B-1050 Brussels, Belgium
10Department of Physics, Chiba University, Chiba 263-8522, Japan
11Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
12Department of Physics, University of Maryland, College Park, Maryland 20742, USA
13Department of Physics, Universität Dortmund, D-44221 Dortmund, Germany
14Department of Subatomic and Radiation Physics, University of Gent, B-9000 Gent, Belgium
15Max-Planck-Institut für Kernphysik, D-69177 Heidelberg, Germany
16Department of Physics and Astronomy, University of California, Irvine, California 92697, USA
17Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045, USA
18Blackett Laboratory, Imperial College, London SW7 2BW, United Kingdom
19Department of Astronomy, University of Wisconsin, Madison, Wisconsin 53706, USA
20Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA
21Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz, Germany
22University of Mons-Hainaut, 7000 Mons, Belgium
23Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA
24Department of Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP, United Kingdom
25Institute for Advanced Study, Princeton, New Jersey 08540, USA
26Department of Physics, University of Wisconsin, River Falls, Wisconsin 54022, USA
27Department of Physics, Stockholm University, SE-10691 Stockholm, Sweden
28Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
29Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
30Division of High Energy Physics, Uppsala University, S-75121 Uppsala, Sweden
31Department of Physics and Astronomy, Utrecht University/SRON, NL-3584 CC Utrecht, The Netherlands
32Department of Physics, University of Wuppertal, D-42119 Wuppertal, Germany
33DESY, D-15735 Zeuthen, Germany
Received 24 April 2007; published 31 August 2007
A search for TeV-PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collected between 2000 and 2003 with an equivalent live time of 807 days. This diffuse analysis sought to find an extraterrestrial neutrino flux from sources with nonthermal components. The signal is expected to have a harder spectrum than the atmospheric muon and neutrino backgrounds. Since no excess of events was seen in the data over the expected background, an upper limit of E2Phi90%C.L.<7.4×10-8 GeV cm-2 s-1 sr-1 is placed on the diffuse flux of muon neutrinos with a Phi[proportional]E-2 spectrum in the energy range 16 TeV to 2.5 PeV. This is currently the most sensitive Phi[proportional]E-2 diffuse astrophysical neutrino limit. We also set upper limits for astrophysical and prompt neutrino models, all of which have spectra different from Phi[proportional]E-2.
©2007 The American Physical Society
| URL: |
http://link.aps.org/doi/10.1103/PhysRevD.76.042008
|
| DOI: |
10.1103/PhysRevD.76.042008 |
| PACS: |
95.55.Vj;
95.75.-z;
95.85.Ry
|
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