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Search for heavy isosinglet neutrinos

✍ Scribed by P. Vilain; G. Wilquet; S. Petrak; R. Beyer; W. Flegel; H. Grote; T. Mouthuy; H. Øveras; J. Panman; K. Winter; G. Zacek; V. Zacek; F.W. Büsser; C. Foos; L. Gerland; T. Layda; F. Niebergall; G. Rädel; P. Stähelin; T. Voss; D. Favart; G. Grégoire; E. Knoops; V. Lemaître; P. Gorbunov; E. Grigoriev; V. Khovansky; A. Maslennikov; A. Rozanov; W. Lippich; A. Nathaniel; A. Staude; J. Vogt; A.G. Cocco; A. Ereditato; G. Fiorillo; F. Marchetti-Stasi; V. Palladino; P. Strolin; A. Capone; D. De Pedis; U. Dore; A. Frenkel-Rambaldi; P.F. Loverre; D. Macina; G. Piredda; R. Santacesaria; E. Di Capua; S. Ricciardi; B. Saitta; B. Akkus; E. Arik; M. Serin-Zeyrek; R. Sever; P. Tolun; K. Hiller; R. Nahnhauer; H.E. Roloff


Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
580 KB
Volume
351
Category
Article
ISSN
0370-2693

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Search for heavy isosinglet neutrinos
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With completion expected in 2011, the IceCube Neutrino Observatory is approaching the 1 km 3 scale required for high energy neutrino astronomy. Before completion, the data taken with the deployed strings of the IceCube detector allows the testing of different procedures of searching for high energy