Updated results from the ν(τ) appearance search in NOMAD

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; A. Bunyatov; L. Camilleri; A. Cardini; P. W. Cattaneo; V. Cavasinni; A. Cervera-Villanueva; G. Collazuol; G. Conforto; C. Conta; M. Contalbrigo; R. Cousins; D. Daniels; H. Degaudenzi; Del Prete; A. De Santo; T. Dignan; A. Di Lella; E. do Couto e Silva; J. Dumarchez; M. Ellis; G. J. Feldman; 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. Guglielm; 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; V. E. Kuznetsov; S. Lacaprara; C. Lachaud; B. Lakic; A. Lanza; 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; Y. 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; L. Rebuffi; J. Rico; C. Roda; A. Rubbia; F. Salvatore; K. Schahmaneche; B. Schmidt; M. Sevior; D. Sillou; F. J.P. Soler; G. Sozzi; D. Steele; M. Steininger; 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; J. M. Vieira; T. Vinogradova; F. V. Weber; T. Weisse; F. F. Wilson; L. J. Winton; B. D. Yabsley; H. Zaccone; K. Zuber; P. Zuccon

doi:10.1016/S0370-2693(00)00611-0

Updated results from the ν(τ) appearance search in NOMAD

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, A. Bunyatov, L. Camilleri, A. Cardini, P. W. Cattaneo, V. Cavasinni, A. Cervera-VillanuevaG. Collazuol, G. Conforto, C. Conta, M. Contalbrigo, R. Cousins, D. Daniels, H. Degaudenzi, Del Prete, A. De Santo, T. Dignan, A. Di Lella, E. do Couto e Silva, J. Dumarchez, M. Ellis, G. J. Feldman, 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. Guglielm, 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, V. E. Kuznetsov, S. Lacaprara, C. Lachaud, B. Lakic, A. Lanza, 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, Y. 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, L. Rebuffi, J. Rico, C. Roda, A. Rubbia, F. Salvatore, K. Schahmaneche, B. Schmidt, M. Sevior, D. Sillou, F. J.P. Soler, G. Sozzi, D. Steele, M. Steininger, 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, J. M. Vieira, T. Vinogradova, F. V. Weber, T. Weisse, F. F. Wilson, L. J. Winton, B. D. Yabsley, H. Zaccone, K. Zuber, P. Zuccon

Research output: Contribution to journal › Article › peer-review

20 Scopus citations

Abstract

Updated results from the appearance searches for ν(υ) → ν(τ) and ν(e) → ν(τ) oscillations in the full NOMAD data sample are reported. The increased data and the use of more refined kinematic schemes for the ν(τ) CC selection allow a significant improvement of the overall sensitivity. The 'blind analysis' of both the deep-inelastic and the low multiplicity samples yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% C.L. region in the sin ² 2θ(μτ) - Δm ² plane which includes sin ² 2θ(μτ) < 4.4 x 10 ^-4 at large Δm ² and Δm ² <0.8 eV ² /c ⁴ at sin ² 2θ(μτ) = 1. The corresponding contour in the v(e) → ν(τ) oscillation hypothesis results in sin ² 2θ(eτ) < 2.2 x 10 ^-2 at large Δm ² and Δm ² <6.5 eV ² /c ⁴ at sin ² 2θ(eτ) = 1. (C) 2000 Elsevier Science B.V.

Original language	English (US)
Pages (from-to)	387-404
Number of pages	18
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	483
Issue number	4
DOIs	https://doi.org/10.1016/S0370-2693(00)00611-0
State	Published - Jun 22 2000
Externally published	Yes

Keywords

Neutrino oscillations

ASJC Scopus subject areas

Nuclear and High Energy Physics

Access to Document

10.1016/S0370-2693(00)00611-0

Cite this

Autiero, D., Baldisseri, A., Baldo-Ceolin, M., Ballocchi, G., Banner, M., Bassompierre, G., Benslama, K., Besson, N., Bird, I., Blumenfeld, B., Bobisut, F., Bouchez, J., Boyd, S., Bueno, A., Bunyatov, A., Camilleri, L., Cardini, A., Cattaneo, P. W., Cavasinni, V., ... Zuccon, P. (2000). Updated results from the ν(τ) appearance search in NOMAD. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 483(4), 387-404. https://doi.org/10.1016/S0370-2693(00)00611-0

Autiero, D, Baldisseri, A, Baldo-Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, A, Camilleri, L, Cardini, A, Cattaneo, PW, Cavasinni, V, Cervera-Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Prete, D, De Santo, A, Dignan, T, Di Lella, A, do Couto e Silva, E, Dumarchez, J, Ellis, M, Feldman, GJ, Ferrari, R, Ferrère, D, Flaminio, V, Fraternali, M, Gaillard, JM, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez-Cadenas, JJ, Gosset, J, Gößling, C, Gouanère, M, Grant, A, Graziani, G, Guglielm, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, VE, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, Rotonda, L, Laveder, M, Letessier-Selvon, A, Levy, JM, Linssen, L, Ljubičić, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Méchain, X, Mendiburu, JP, Meyer, JP, Mezzetto, M, Mishra, SR, Moorhead, GF, Nédélec, P, Nefedov, Y, Nguyen-Mau, C, Orestano, D, Pastore, F, Peak, LS, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rebuffi, L, Rico, J, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Sevior, M, Sillou, D, Soler, FJP, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipčević, M, Stolarczyk, TH, Tareb-Reyes, M, Taylor, GN, Tereshchenko, V, Toropin, A, Touchard, AM, Tovey, SN, Tran, MT, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata-Nappi, M, Valuev, V, Vannucci, F, Varvell, KE, Veltri, M, Vercesi, V, Vieira, JM, Vinogradova, T, Weber, FV, Weisse, T, Wilson, FF, Winton, LJ, Yabsley, BD, Zaccone, H, Zuber, K & Zuccon, P 2000, 'Updated results from the ν(τ) appearance search in NOMAD', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 483, no. 4, pp. 387-404. https://doi.org/10.1016/S0370-2693(00)00611-0

@article{6d89296c984d4f89996140f6b7ec49f7,

title = "Updated results from the ν(τ) appearance search in NOMAD",

abstract = " Updated results from the appearance searches for ν(υ) → ν(τ) and ν(e) → ν(τ) oscillations in the full NOMAD data sample are reported. The increased data and the use of more refined kinematic schemes for the ν(τ) CC selection allow a significant improvement of the overall sensitivity. The 'blind analysis' of both the deep-inelastic and the low multiplicity samples yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% C.L. region in the sin 2 2θ(μτ) - Δm 2 plane which includes sin 2 2θ(μτ) < 4.4 x 10 -4 at large Δm 2 and Δm 2 <0.8 eV 2 /c 4 at sin 2 2θ(μτ) = 1. The corresponding contour in the v(e) → ν(τ) oscillation hypothesis results in sin 2 2θ(eτ) < 2.2 x 10 -2 at large Δm 2 and Δm 2 <6.5 eV 2 /c 4 at sin 2 2θ(eτ) = 1. (C) 2000 Elsevier Science B.V. ",

keywords = "Neutrino oscillations",

author = "D. Autiero and A. Baldisseri and M. Baldo-Ceolin and G. Ballocchi and M. Banner and G. Bassompierre and K. Benslama and N. Besson and I. Bird and B. Blumenfeld and F. Bobisut and J. Bouchez and S. Boyd and A. Bueno and A. Bunyatov and L. Camilleri and A. Cardini and Cattaneo, {P. W.} and V. Cavasinni and A. Cervera-Villanueva and G. Collazuol and G. Conforto and C. Conta and M. Contalbrigo and R. Cousins and D. Daniels and H. Degaudenzi and Del Prete and {De Santo}, A. and T. Dignan and {Di Lella}, A. and {do Couto e Silva}, E. and J. Dumarchez and M. Ellis and Feldman, {G. J.} and R. Ferrari and D. Ferr{\`e}re and V. Flaminio and M. Fraternali and Gaillard, {J. M.} and E. Gangler and A. Geiser and D. Geppert and D. Gibin and S. Gninenko and A. Godley and Gomez-Cadenas, {J. J.} and J. Gosset and C. G{\"o}{\ss}ling and M. Gouan{\`e}re and A. Grant and G. Graziani and A. Guglielm and C. Hagner and J. Hernando and D. Hubbard and P. Hurst and N. Hyett and E. Iacopini and C. Joseph and F. Juget and M. Kirsanov and O. Klimov and J. Kokkonen and A. Kovzelev and A. Krasnoperov and Kuznetsov, {V. E.} and S. Lacaprara and C. Lachaud and B. Lakic and A. Lanza and La Rotonda and M. Laveder and A. Letessier-Selvon and Levy, {J. M.} and L. Linssen and A. Ljubi{\v c}i{\'c} and J. Long and A. Lupi and A. Marchionni and F. Martelli and X. M{\'e}chain and Mendiburu, {J. P.} and Meyer, {J. P.} and M. Mezzetto and Mishra, {S. R.} and Moorhead, {G. F.} and P. N{\'e}d{\'e}lec and Y. Nefedov and C. Nguyen-Mau and D. Orestano and F. Pastore and Peak, {L. S.} and E. Pennacchio and H. Pessard and R. Petti and A. Placci and G. Polesello and D. Pollmann and A. Polyarush and B. Popov and C. Poulsen and L. Rebuffi and J. Rico and C. Roda and A. Rubbia and F. Salvatore and K. Schahmaneche and B. Schmidt and M. Sevior and D. Sillou and Soler, {F. J.P.} and G. Sozzi and D. Steele and M. Steininger and U. Stiegler and M. Stip{\v c}evi{\'c} and TH Stolarczyk and M. Tareb-Reyes and Taylor, {G. N.} and V. Tereshchenko and A. Toropin and Touchard, {A. M.} and Tovey, {S. N.} and Tran, {M. T.} and E. Tsesmelis and J. Ulrichs and L. Vacavant and M. Valdata-Nappi and V. Valuev and F. Vannucci and Varvell, {K. E.} and M. Veltri and V. Vercesi and Vieira, {J. M.} and T. Vinogradova and Weber, {F. V.} and T. Weisse and Wilson, {F. F.} and Winton, {L. J.} and Yabsley, {B. D.} and H. Zaccone and K. Zuber and P. Zuccon",

note = "Funding Information: We thank the management and staff of CERN and of all participating institutes for their vigorous support of the experiment. Particular thanks are due to the CERN accelerator and beam-line staff for the magnificent performance of the neutrino beam. The following funding agencies have contributed to this experiment: Australian Research Council (ARC) and Department of Industry, Science, and Resources (DISR), Australia; Institut National de Physique Nucl{\'e}aire et Physique des Particules (IN2P3), Commissariat {\`a} l'Energie Atomique (CEA), Minist{\`e}re de l'Education Nationale, de l'Enseignement Sup{\'e}rieur et de la Recherche, France; Bundesministerium f{\"u}r Bildung und Forschung (BMBF, contract 05 6DO52), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Russian Foundation for Basic Research, Institute for Nuclear Research of the Russian Academy of Sciences, Russia; Fonds National Suisse de la Recherche Scientifique, Switzerland; Department of Energy, National Science Foundation (grant PHY-9526278), the Sloan and the Cottrell Foundations, USA. F.J.P. Soler is supported by a TMR Fellowship from the European Commission. We also thank our secretarial staff, Jane Barney, Marie-Anne Huber, Rachel Phillips and Mabel Richtering, and the following people who have worked with the collaboration on the preparation and the data collection stages of NOMAD: M. Anfreville, M. Authier, G. Barichello, A. Beer, V. Bonaiti, A. Castera, A. Cavestro, O. Clou{\'e}, C. D{\'e}traz, L. Dumps, C. Engster, G. Fumagalli, G. Gallay, W. Huta, E. Lessmann, J. Mulon, J.P. Pass{\'e}rieux, P. Petitpas, J. Poinsignon, C. Sobczynski, S. Souli{\'e}, L. Visentin, P. Wicht.",

year = "2000",

month = jun,

day = "22",

doi = "10.1016/S0370-2693(00)00611-0",

language = "English (US)",

volume = "483",

pages = "387--404",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

issn = "0370-2693",

publisher = "Elsevier",

number = "4",

}

TY - JOUR

T1 - Updated results from the ν(τ) appearance search in NOMAD

AU - Autiero, D.

AU - Baldisseri, A.

AU - Baldo-Ceolin, M.

AU - Ballocchi, G.

AU - Banner, M.

AU - Bassompierre, G.

AU - Benslama, K.

AU - Besson, N.

AU - Bird, I.

AU - Blumenfeld, B.

AU - Bobisut, F.

AU - Bouchez, J.

AU - Boyd, S.

AU - Bueno, A.

AU - Bunyatov, A.

AU - Camilleri, L.

AU - Cardini, A.

AU - Cattaneo, P. W.

AU - Cavasinni, V.

AU - Cervera-Villanueva, A.

AU - Collazuol, G.

AU - Conforto, G.

AU - Conta, C.

AU - Contalbrigo, M.

AU - Cousins, R.

AU - Daniels, D.

AU - Degaudenzi, H.

AU - Prete, Del

AU - De Santo, A.

AU - Dignan, T.

AU - Di Lella, A.

AU - do Couto e Silva, E.

AU - Dumarchez, J.

AU - Ellis, M.

AU - Feldman, G. J.

AU - Ferrari, R.

AU - Ferrère, D.

AU - Flaminio, V.

AU - Fraternali, M.

AU - Gaillard, J. M.

AU - Gangler, E.

AU - Geiser, A.

AU - Geppert, D.

AU - Gibin, D.

AU - Gninenko, S.

AU - Godley, A.

AU - Gomez-Cadenas, J. J.

AU - Gosset, J.

AU - Gößling, C.

AU - Gouanère, M.

AU - Grant, A.

AU - Graziani, G.

AU - Guglielm, A.

AU - Hagner, C.

AU - Hernando, J.

AU - Hubbard, D.

AU - Hurst, P.

AU - Hyett, N.

AU - Iacopini, E.

AU - Joseph, C.

AU - Juget, F.

AU - Kirsanov, M.

AU - Klimov, O.

AU - Kokkonen, J.

AU - Kovzelev, A.

AU - Krasnoperov, A.

AU - Kuznetsov, V. E.

AU - Lacaprara, S.

AU - Lachaud, C.

AU - Lakic, B.

AU - Lanza, A.

AU - Rotonda, La

AU - Laveder, M.

AU - Letessier-Selvon, A.

AU - Levy, J. M.

AU - Linssen, L.

AU - Ljubičić, A.

AU - Long, J.

AU - Lupi, A.

AU - Marchionni, A.

AU - Martelli, F.

AU - Méchain, X.

AU - Mendiburu, J. P.

AU - Meyer, J. P.

AU - Mezzetto, M.

AU - Mishra, S. R.

AU - Moorhead, G. F.

AU - Nédélec, P.

AU - Nefedov, Y.

AU - Nguyen-Mau, C.

AU - Orestano, D.

AU - Pastore, F.

AU - Peak, L. S.

AU - Pennacchio, E.

AU - Pessard, H.

AU - Petti, R.

AU - Placci, A.

AU - Polesello, G.

AU - Pollmann, D.

AU - Polyarush, A.

AU - Popov, B.

AU - Poulsen, C.

AU - Rebuffi, L.

AU - Rico, J.

AU - Roda, C.

AU - Rubbia, A.

AU - Salvatore, F.

AU - Schahmaneche, K.

AU - Schmidt, B.

AU - Sevior, M.

AU - Sillou, D.

AU - Soler, F. J.P.

AU - Sozzi, G.

AU - Steele, D.

AU - Steininger, M.

AU - Stiegler, U.

AU - Stipčević, M.

AU - Stolarczyk, TH

AU - Tareb-Reyes, M.

AU - Taylor, G. N.

AU - Tereshchenko, V.

AU - Toropin, A.

AU - Touchard, A. M.

AU - Tovey, S. N.

AU - Tran, M. T.

AU - Tsesmelis, E.

AU - Ulrichs, J.

AU - Vacavant, L.

AU - Valdata-Nappi, M.

AU - Valuev, V.

AU - Vannucci, F.

AU - Varvell, K. E.

AU - Veltri, M.

AU - Vercesi, V.

AU - Vieira, J. M.

AU - Vinogradova, T.

AU - Weber, F. V.

AU - Weisse, T.

AU - Wilson, F. F.

AU - Winton, L. J.

AU - Yabsley, B. D.

AU - Zaccone, H.

AU - Zuber, K.

AU - Zuccon, P.

N1 - Funding Information: We thank the management and staff of CERN and of all participating institutes for their vigorous support of the experiment. Particular thanks are due to the CERN accelerator and beam-line staff for the magnificent performance of the neutrino beam. The following funding agencies have contributed to this experiment: Australian Research Council (ARC) and Department of Industry, Science, and Resources (DISR), Australia; Institut National de Physique Nucléaire et Physique des Particules (IN2P3), Commissariat à l'Energie Atomique (CEA), Ministère de l'Education Nationale, de l'Enseignement Supérieur et de la Recherche, France; Bundesministerium für Bildung und Forschung (BMBF, contract 05 6DO52), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Russian Foundation for Basic Research, Institute for Nuclear Research of the Russian Academy of Sciences, Russia; Fonds National Suisse de la Recherche Scientifique, Switzerland; Department of Energy, National Science Foundation (grant PHY-9526278), the Sloan and the Cottrell Foundations, USA. F.J.P. Soler is supported by a TMR Fellowship from the European Commission. We also thank our secretarial staff, Jane Barney, Marie-Anne Huber, Rachel Phillips and Mabel Richtering, and the following people who have worked with the collaboration on the preparation and the data collection stages of NOMAD: M. Anfreville, M. Authier, G. Barichello, A. Beer, V. Bonaiti, A. Castera, A. Cavestro, O. Cloué, C. Détraz, L. Dumps, C. Engster, G. Fumagalli, G. Gallay, W. Huta, E. Lessmann, J. Mulon, J.P. Passérieux, P. Petitpas, J. Poinsignon, C. Sobczynski, S. Soulié, L. Visentin, P. Wicht.

PY - 2000/6/22

Y1 - 2000/6/22

N2 - Updated results from the appearance searches for ν(υ) → ν(τ) and ν(e) → ν(τ) oscillations in the full NOMAD data sample are reported. The increased data and the use of more refined kinematic schemes for the ν(τ) CC selection allow a significant improvement of the overall sensitivity. The 'blind analysis' of both the deep-inelastic and the low multiplicity samples yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% C.L. region in the sin 2 2θ(μτ) - Δm 2 plane which includes sin 2 2θ(μτ) < 4.4 x 10 -4 at large Δm 2 and Δm 2 <0.8 eV 2 /c 4 at sin 2 2θ(μτ) = 1. The corresponding contour in the v(e) → ν(τ) oscillation hypothesis results in sin 2 2θ(eτ) < 2.2 x 10 -2 at large Δm 2 and Δm 2 <6.5 eV 2 /c 4 at sin 2 2θ(eτ) = 1. (C) 2000 Elsevier Science B.V.

AB - Updated results from the appearance searches for ν(υ) → ν(τ) and ν(e) → ν(τ) oscillations in the full NOMAD data sample are reported. The increased data and the use of more refined kinematic schemes for the ν(τ) CC selection allow a significant improvement of the overall sensitivity. The 'blind analysis' of both the deep-inelastic and the low multiplicity samples yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% C.L. region in the sin 2 2θ(μτ) - Δm 2 plane which includes sin 2 2θ(μτ) < 4.4 x 10 -4 at large Δm 2 and Δm 2 <0.8 eV 2 /c 4 at sin 2 2θ(μτ) = 1. The corresponding contour in the v(e) → ν(τ) oscillation hypothesis results in sin 2 2θ(eτ) < 2.2 x 10 -2 at large Δm 2 and Δm 2 <6.5 eV 2 /c 4 at sin 2 2θ(eτ) = 1. (C) 2000 Elsevier Science B.V.

KW - Neutrino oscillations

UR - http://www.scopus.com/inward/record.url?scp=0034702158&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0034702158&partnerID=8YFLogxK

U2 - 10.1016/S0370-2693(00)00611-0

DO - 10.1016/S0370-2693(00)00611-0

M3 - Article

AN - SCOPUS:0034702158

VL - 483

SP - 387

EP - 404

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 4

ER -

Updated results from the ν(τ) appearance search in NOMAD

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