The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

The muon and anti-muon neutrino energy spectrum is determined from 2000–2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2–200 TeV. The result is compared to different atmospheric neutrino models and it is compatible w...

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Veröffentlicht in:Astroparticle physics 2010-08, Vol.34 (1), p.48-58
Hauptverfasser: Abdou, Y., Baker, M., Bay, R., Becker, J.K., Becker, K.-H., Berdermann, J., Berghaus, P., Bertrand, D., Blaufuss, E., Böser, S., Bradley, L., Christy, B., Clem, J., Cowen, D.F., Danninger, M., De Clercq, C., Descamps, F., DeYoung, T., Dreyer, J., Dumm, J.P., Duvoort, M.R., Ehrlich, R., Eisch, J., Euler, S., Fadiran, O., Fazely, A.R., Foerster, M.M., Fox, B.D., Franke, R., Gaisser, T.K., Gladstone, L., Glüsenkamp, T., Goodman, J.A., Griesel, T., Gunasingha, R.M., Gurtner, M., Halzen, F., Han, K., Hickford, S., Hill, G.C., Hoffman, K.D., Hoshina, K., Huelsnitz, W., Hülß, J.-P., Hultqvist, K., Hussain, S., Imlay, R.L., Jacobsen, J., Japaridze, G.S., Johansson, H., Joseph, J.M., Kenny, P., Kohnen, G., Kowalski, M., Krings, T., Kroll, G., Lafebre, S., Landsman, H., Madsen, J., Mase, K., Matis, H.S., Matusik, M., Milke, N., Movit, S.M., Nießen, P., Nygren, D.R., Odrowski, S., Olivo, M., Ono, M., Panknin, S., Paul, L., Petrovic, J., Pieloth, D., Porrata, R., Rhode, W., Ryckbosch, D., Schatto, K., Schunck, M., Silvestri, A., Stephens, G., Stezelberger, T., Stokstad, R.G., Stoyanov, S., Tamburro, A., Tepe, A., Ter-Antonyan, S., Toale, P.A., Tosi, D., Turčan, D., van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., van Santen, J., Whitehorn, N., Wischnewski, R., Wissing, H., Woschnagg, K., Xu, X.W., Yoshida, S., Zarzhitsky, P.
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Sprache:eng
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Zusammenfassung:The muon and anti-muon neutrino energy spectrum is determined from 2000–2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2–200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.
ISSN:0927-6505
1873-2852
1873-2852
DOI:10.1016/j.astropartphys.2010.05.001