The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector
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Authors
Abbasi, R.
Abdou, Y.
Abu-Zayyad, T.
Adams, J.
Aguilar, J.
Ahlers, M.
Andeen, K.
Auffenberg, J.
Bai, X.
Baker, M.
Barwick, S.
Bay, R.
Bazo Alba, J.
Beattie, K.
Beatty, J.
Bechet, S.
Becker, J.
Becker, K.
Benabderrahmane, M.
Berdermann, J.
Berghaus, P.
Berley, D.
Bernardini, E.
Bertrand, D.
Besson, D.
Bissok, M.
Blaufuss, E.
Boersma, D.
Bohm, C.
Böser, S.
Botner, O.
Bradley, L.
Braun, J.
Buitink, S.
Carson, Michael
Chirkin, D.
Christy, B.
Clem, J.
Clevermann, F.
Cohen, S.
Colnard, C.
Cowen, D.
D'Agostino, M.
Danninger, M.
De Clercq, C.
Demirörs, L.
Depaepe, O.
Descamps, F.
Desiati, P.
De Vries-Uiterweerd, G.
Deyoung, T.
Díaz-Vélez, J.
Dreyer, J.
Dumm, J.
Duvoort, M.
Ehrlich, R.
Eisch, J.
Ellsworth, R.
Engdegrd, O.
Euler, S.
Evenson, P.
Fadiran, O.
Fazely, A.
Fedynitch, A.
Feusels, T.
Filimonov, K.
Finley, C.
Foerster, M.
Fox, B.
Franckowiak, A.
Franke, R.
Gaisser, T.
Gallagher, J.
Ganugapati, R.
Geisler, M.
Gerhardt, L.
Gladstone, L.
Glüsenkamp, T.
Goldschmidt, A.
Goodman, J.
Grant, D.
Griesel, T.
Groß, A.
Grullon, S.
Gunasingha, R.
Gurtner, M.
Ha, C.
Hallgren, A.
Halzen, F.
Han, K.
Hanson, K.
Helbing, K.
Herquet, P.
Hickford, S.
Hill, G.
Hoffman, K.
Date
2010Type
Journal Article
Metadata
Show full item recordCitation
Abbasi, R. and Abdou, Y. and Abu-Zayyad, T. and Adams, J. and Aguilar, J. and Ahlers, M. and Andeen, K. et al. 2010. The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector. Astroparticle Physics. 34 (1): pp. 48-58.
Source Title
Astroparticle Physics
ISSN
School
Department of Exploration Geophysics
Collection
Abstract
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.
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