A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A (0.83 × 2π) sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an E−2 flux spectrum, a 90% c.l. upper limit on the diffuse νμ flux of E2Φ90% = 5.3 × 10−8 GeVcm−2 s−1 sr−1 in the energy range 20 TeV–2.5 PeV is obtained. Other signal models with different energy spectra are also tested and some rejected.

Search for a diffuse flux of high-energy muon neutrino with the ANTARES neutrino telescope

BAZZOTTI, MARCO;BIAGI, SIMONE;CARMINATI, GIADA;CECCHINI, STEFANO;CHIARUSI, TOMMASO;GIACOMELLI, GIORGIO MARIA;MARGIOTTA, ANNARITA;SPURIO, MAURIZIO;
2011

Abstract

A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A (0.83 × 2π) sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an E−2 flux spectrum, a 90% c.l. upper limit on the diffuse νμ flux of E2Φ90% = 5.3 × 10−8 GeVcm−2 s−1 sr−1 in the energy range 20 TeV–2.5 PeV is obtained. Other signal models with different energy spectra are also tested and some rejected.
J.A. Aguilar ; I. Al Samarai ; A. Albert; M. André ; M. Anghinolfi ; G. Anton; S. Anvar; M. Ardid; A.C. Assis Jesus ; T. Astraatmadj; J.-J. Aubert; R. Auer ; B. Baret; S. Basa; M. Bazzotti; V. Bertin; S. Biagi; C. Bigongiari ; C. Bogazzi ; M. Bou-Cabo; M.C. Bouwhuis ; A.M. Brown; J. Brunner; J. Busto ; F. Camarena ; A. Capone; C. Cârloganu; G. Carminati; J. Carr; S. Cecchini; Ph. Charvis ; T. Chiarusi; M. Circella ; R. Coniglione ; H. Costantini ; N. Cottini ; P. Coyle; C. Curtil; M.P. Decowski ; I. Dekeyser; A. Deschamps; C. Donzaud; D. Dornic ; Q. Dorosti ; D. Drouhin; T. Eberl ; U. Emanuele ; J.-P. Ernenwein ; S. Escoffier ; F. Fehr; V. Flaminio; F. Folger; U. Fritsch; J.-L. Fuda ; S. Galata ; P. Gay; G. Giacomelli; J.P. Gómez-González ; K. Graf; G. Guillard ; G. Halladjian ; G. Hallewell ; H. van Haren; A.J. Heijboer; Y. Hello ; J.J. Hernández-Rey ; B. Herold; J. Hößl ; C.C. Hsu; M. de Jon; M. Kadler; N. Kalantar-Nayestanaki ; O. Kalekin; A. Kappes; U. Katz ; P. Kooijman ; C. Kopper ; A. Kouchner ; V. Kulikovskiy ; R. Lahmann; P. Lamar ; G. Larosa ; D. Lefèvre ; G. Lim; D. Lo Presti; H. Loehner ; S. Loucatos; F. Lucarelli; S. Mangano; M. Marcelin ; A. Margiotta; J.A. Martinez-Mora; A. Mazure; A. Meli ; T. Montaruli; M. Morganti; L. Moscoso; H. Motz; C. Naumann; M. Neff; D. Palioselitis; G.E. Pa˘va˘las¸ ; P. Payre ; J. Petrovic ; P. Piattelli ; N. Picot-Clemente ; C. Picq ; V. Popa; T. Pradier; E. Presani; C. Racca ; C. Reed ; G. Riccobene ; C. Richardt ; K. Roensch; A. Rostovtsev ; M. Rujoiu; G.V. Russo ; F. Salesa; P. Sapienza ; F. Schöck; J.-P. Schuller ; R. Shanidze ; F. Simeone; A. Spies; M. Spurio; J.J.M. Steijger ; Th. Stolarczyk ; M. Taiuti ; C. Tamburini ; L. Tasca; S. Toscano ; B. Vallage ; V. Van Elewyck ; G. Vannoni ; M. Vecchi; P. Vernin ; G. Wijnker ; E. de Wolf; H. Yepes ; D. Zaborov ; J.D. Zornoza ; J. Zúñiga
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11585/97315
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