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Prediction of neutrino fluxes in the NOMAD experiment

✍ Scribed by P Astier; D Autiero; A Baldisseri; M Baldo-Ceolin; M Banner; G Bassompierre; K Benslama; N Besson; I Bird; B Blumenfeld; F Bobisut; J Bouchez; S Boyd; A Bueno; S Bunyatov; L Camilleri; A Cardini; P.W Cattaneo; V Cavasinni; A Cervera-Villanueva; G Collazuol; G Conforto; C Conta; R Cousins; D Daniels; H Degaudenzi; T Del Prete; A De Santo; T Dignan; L Di Lella; E do Couto e Silva; J Dumarchez; M Ellis; G.J Feldman; A Ferrari; R Ferrari; D Ferrère; V Flaminio; M Fraternali; J.-M Gaillard; E Gangler; A Geiser; D Geppert; D Gibin; S Gninenko; A Godley; J.-J Gomez-Cadenas; J Gosset; C Gößling; M Gouanère; A Grant; G Graziani; A Guglielmi; C Hagner; J Hernando; T.M Hong; D Hubbard; P Hurst; N Hyett; E Iacopini; C Joseph; F Juget; M Kirsanov; O Klimov; J Kokkonen; A Kovzelev; A Krasnoperov; C Lachaud; B Lakić; A Lanza; L La Rotonda; M Laveder; A Letessier-Selvon; J.-M Levy; L Linssen; A Ljubičić; J Long; A Lupi; A Marchionni; F Martelli; X Méchain; J.-P Mendiburu; J.-P Meyer; M Mezzetto; S.R Mishra; G.F Moorhead; P Nédélec; Yu Nefedov; C Nguyen-Mau; D Orestano; F Pastore; L.S Peak; E Pennacchio; H Pessard; R Petti; A Placci; G Polesello; D Pollmann; A Polyarush; B Popov; C Poulsen; J Rico; P Riemann; C Roda; A Rubbia; F Salvatore; K Schahmaneche; B Schmidt; T Schmidt; M Sevior; D Shih; D Sillou; F.J.P Soler; G Sozzi; D Steele; U Stiegler; M Stipčević; Th Stolarczyk; M Tareb-Reyes; G.N Taylor; V Tereshchenko; A Toropin; A.-M Touchard; S.N Tovey; M.-T Tran; E Tsesmelis; J Ulrichs; L Vacavant; M Valdata-Nappi; V Valuev; F Vannucci; K.E Varvell; M Veltri; V Vercesi; G Vidal-Sitjes; J.-M Vieira; T Vinogradova; F.V Weber; T Weisse; F.F Wilson; L.J Winton; B.D Yabsley; H Zaccone; K Zuber


Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
547 KB
Volume
515
Category
Article
ISSN
0168-9002

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✍ M. Honda 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 434 KB

The uncertainty in the calculation of atmospheric neutrino fluxes is studied. The absolute value of atmospheric neutrino fluxes is sensitive to variation of the primary cosmic ray flux model asld/or the interaction model. However, the ratios between different kind of neutrinos stay almost unchanged