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Measurement of the atmospheric $\nu_\mu$ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

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arxiv 1308.1599 v1 pith:QPA2WYXF submitted 2013-08-07 astro-ph.HE astro-ph.IM

The ANTARES Collaboration , S. Adrián-Martínez , A. Albert , I. Al Samarai , M. André , M. Anghinolfi , G. Anton , S. Anvar
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M. Ardid T. Astraatmadja J-J. Aubert B. Baret J. Barrios-Martí S. Basa V. Bertin S. Biagi C. Bigongiari C. Bogazzi B. Bouhou M.C. Bouwhuis R. Bruijn J. Brunner J. Busto A. Capone L. Caramete C. Carloganu J. Carr S. Cecchini Z. Charif Ph. Charvis T. Chiarusi M. Circella F. Classen L. Core H. Costantini P. Coyle A. Creusot C. Curtil I. Dekeyser A. Deschamps G. De Bonis M.P. Decowski C. Distefano C. Donzaud D. Dornic Q. Dorosti D. Drouhin A. Dumas T. Eberl U. Emanuele A. Enzenhöfer J-P. Ernenwein S. Escoffier K. Fehn P. Fermani V. Flaminio F. Folger U. Fritsch L.A. Fusco S. Galatà P. Gay S. Geisselsöder K. Geyer G. Giacomelli V. Giordano A. Gleixner J.P. Gómez-González K. Graf G. Guillard H. van Haren A.J. Heijboer Y. Hello J.J. Hernández-Rey B. Herold J. Hössl C.W. James M. de Jong M. Kadler O. Kalekin A. Kappes U. Katz P. Kooijman A. Kouchner I. Kreykenbohm V. Kulikovskiy R. Lahmann E. Lambard G. Lambard G. Larosa D. Lattuada D. Lefèvre E. Leonora D. Lo Presti H. Loehner S. Loucatos F. Louis S. Mangano M. Marcelin A. Margiotta J.A. Martínez-Mora S. Martini T. Michael T. Montaruli M. Morganti H. Motz C. Mueller M. Neff E. Nezri D. Palioselitis G.E. Pavalas C. Perrina P. Piattelli V. Popa T. Pradier C. Racca R. Richter C. Rivière A. Robert K. Roensch A. Rostovtsev D. F. E. Samtleben M. Sanguineti P. Sapienza J. Schmid J. Schnabel S. Schulte F. Schüssler T. Seitz R. Shanidze C. Sieger F. Simeone A. Spies M. Spurio J.J.M. Steijger Th. Stolarczyk A. Sánchez-Losa M. Taiuti C. Tamburini Y. Tayalati A. Trovato B. Vallage C. Vallée V. Van Elewyck P. Vernin E. Visser S. Wagner J. Wilms E. de Wolf K. Yatkin H. Yepes J.D. Zornoza J. Zúñiga
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keywords atmosphericenergyfluxantarescompatiblemeasurementneutrinoneutrinos
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Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric \nu_\mu + \bar{\nu}_\mu energy spectrum in the energy range 0.1 - 200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is ~25% higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index \gamma_{meas}=3.58\pm 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

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    astro-ph.HE 2026-08 accept novelty 5.0 of 10

    Using 640 days of KM3NeT/ARCA data, the collaboration finds no significant diffuse astrophysical neutrino flux and sets upper limits for all-sky and Galactic Ridge emission.

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