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A More Sensitive Search For Nu(Mu) -> Nu(Tau) Oscillations In Nomad

P Astier,D Autiero,A Baldisseri,M Baldo-Ceolin,G Ballocchi,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,Pw Cattaneo,V Cavasinni,A Cervera-Villanueva,G Collazuol,G Conforto,C Conta,M Contalbrigo,R Cousins,D Daniels,H Degaudenzi,T Del Prete,A De Santo,T Dignan,L Di Lella,Ede Silva, Ij Donnelly,J Dumarchez,M Ellis,T Fazio,Gj Feldman,R Ferrari,D Ferrere,V Flaminio,M Fraternali,Jm Gaillard, A Gandolfo,E Gangler,A Geiser,D Geppert,D Gibin,S Gninenko,A Godley,Jj Gomez-Cadenas,J Gosset,C Gossling,M Gouanere,A Grant,G Graziani,A Guglielmi,C Hagner,J Hernando,D Hubbard,P Hurst,N Hyett,E Iacopini,C Joseph,F Juget,M Kirsanov,O Klimov,J Kokkonen,A Kovzelev,A Krasnoperov,Ve Kuznetsov,S Lacaprara,C Lachaud,B Lakic,A Lanza,L La Rotonda,M Laveder,A Letessier-Selvon,Jm Levy,L Linssen, A Ljubicic,J Long, A Lupi,E Manola-Poggioli,A Marchionni,F Martelli,X Mechain,Jp Mendiburu,Jp Meyer,M Mezzetto,Sr Mishra,Gf Moorhead,L Mossuz,P Nedelec,Y Nefedov,C Nguyen-Mau,D Orestano,F Pastore,Ls Peak,E Pennacchio,H Pessard,R Petti,A Placci,A Pluquet,G Polesello,D Pollmann,B Popov,C Poulsen,P Rathouit, R Reno,G Renzoni,J Rico,P Riemann,C Roda,A Rubbia,F Salvatore,K Schahmaneche, B Schmidt,T Schmidt,G Segneri,M Sevior,D Sillou,Fjp Soler,G Sozzi,D Steele,M Steininger,U Stiegler,M Stipcevic,T Stolarczyk, M Tareb-Reyes,Gn Taylor,V Tereshchenko,A Toropin,Am Touchard,Sn Tovey,Mt Tran,E Tsesmelis,J Ulrichs,L Vacavant,M Valdata-Nappi,V Valuev,F Vannucci,Ke Varvell,M Veltri,V Vercesi, D Verkindt,Jm Vieira,T Vinogradova,Mk Vo,S Volkov,Fv Weber,T Weisse,Ff Wilson,Lj Winton,Bd Yabsley,H Zaccone,K Zuber,P Zuccon

PHYSICS LETTERS B(1999)

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摘要
With additional data and improved algorithms, we have enhanced the sensitivity of our appearance search for nu(mu) --> nu(tau) oscillations in the NOMAD detector in the CERN-SPS wide-band neutrino beam. The search uses kinematic criteria to identify nu(tau) charged current interactions followed by decay of the tau(-) to one of several decay modes. Our "blind'' analyses of deep-inelastic scattering data taken in 1996 and 1997, combined with consistent reanalyses of previously reported 1995 data, yield no oscillation signal. For the two-family oscillation scenario, we present the contour outlining a 90% C.L. confidence region in the sin(2)2 theta(mu tau) - Delta m(2) plane. At large Delta m(2) the confidence region includes sin(2)2 theta(mu tau) < 1.2 X 10(-3) (a limit 3.5 times more stringent than in our previous publication), while at sin(2)2 theta(mu tau) = 1 the confidence region includes Delta m(2) < 1.2 eV(2)/c(4). (C) 1999 Published by Elsevier Science B.V. All rights reserved.
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neutrino oscillations
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