Prediction of neutrino fluxes in the NOMAD experiment

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. Göbling; M. Gouanere; 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. Ljubiĉić; J. Long; A. Lupi; A. Marchionni; F. Martelli; X. Mechain; J. P. Mendiburu; J. P. Meyer; M. Mezzetto; S. R. Mishra; G. F. Moorhead; P. Nedelec; 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. Stipĉević; 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

doi:10.1016/j.nima.2003.07.054

Prediction of neutrino fluxes in the NOMAD experiment

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-VillanuevaG. 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. Göbling, M. Gouanere, 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. Ljubiĉić, J. Long, A. Lupi, A. Marchionni, F. Martelli, X. Mechain, J. P. Mendiburu, J. P. Meyer, M. Mezzetto, S. R. Mishra, G. F. Moorhead, P. Nedelec, 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. Stipĉević, 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

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

Abstract

The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for ν_μ and ν_e, 10% for ν̄_μ, and 12% for ν̄ _e. The energy-dependent uncertainty achieved on the ν _e/ν_μ prediction needed for a ν _μ→ν_e oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.

Original language	English (US)
Pages (from-to)	800-828
Number of pages	29
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	515
Issue number	3
DOIs	https://doi.org/10.1016/j.nima.2003.07.054
State	Published - Dec 11 2003
Externally published	Yes

Keywords

Neutrino beam
Neutrino fluxes

ASJC Scopus subject areas

Nuclear and High Energy Physics
Instrumentation

Online availability

10.1016/j.nima.2003.07.054

Library availability

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Astier, P., Autiero, D., Baldisseri, A., Baldo-Ceolin, M., Banner, M., Bassompierre, G., Benslama, K., Besson, N., Bird, I., Blumenfeld, B., Bobisut, F., Bouchez, J., Boyd, S., Bueno, A., Bunyatov, S., Camilleri, L., Cardini, A., Cattaneo, P. W., Cavasinni, V., ... Zuber, K. (2003). Prediction of neutrino fluxes in the NOMAD experiment. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 515(3), 800-828. https://doi.org/10.1016/j.nima.2003.07.054

Astier, P, Autiero, D, Baldisseri, A, Baldo-Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, PW, Cavasinni, V, Cervera-Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, de Santo, A, Dignan, T, di Lella, L, do Couto e Silva, E, Dumarchez, J, Ellis, M, Feldman, GJ, Ferrari, A, 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, Göbling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hong, TM, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Lachaud, C, Lakić, B, Lanza, A, la Rotonda, L, Laveder, M, Letessier-Selvon, A, Levy, JM, Linssen, L, Ljubiĉić, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, JP, Meyer, JP, Mezzetto, M, Mishra, SR, Moorhead, GF, Nedelec, 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, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Shih, D, Sillou, D, Soler, FJP, Sozzi, G, Steele, D, Stiegler, U, Stipĉević, M, Stolarczyk, T, 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, Vidal-Sitjes, G, Vieira, JM, Vinogradova, T, Weber, FV, Weisse, T, Wilson, FF, Winton, LJ, Yabsley, BD, Zaccone, H & Zuber, K 2003, 'Prediction of neutrino fluxes in the NOMAD experiment', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 515, no. 3, pp. 800-828. https://doi.org/10.1016/j.nima.2003.07.054

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title = "Prediction of neutrino fluxes in the NOMAD experiment",

abstract = "The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for νμ and νe, 10% for {\=ν}μ, and 12% for {\=ν} e. The energy-dependent uncertainty achieved on the ν e/νμ prediction needed for a ν μ→νe oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.",

keywords = "Neutrino beam, Neutrino fluxes",

author = "P. Astier and D. Autiero and A. Baldisseri and M. Baldo-Ceolin 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 S. 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 R. Cousins and D. Daniels and H. Degaudenzi and {Del Prete}, T. and {de Santo}, A. and T. Dignan and {di Lella}, L. and {do Couto e Silva}, E. and J. Dumarchez and M. Ellis and Feldman, {G. J.} and A. Ferrari 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}bling and M. Gouanere and A. Grant and G. Graziani and A. Guglielmi and C. Hagner and J. Hernando and Hong, {T. M.} 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 C. Lachaud and B. Laki{\'c} and A. Lanza and {la Rotonda}, L. and M. Laveder and A. Letessier-Selvon and Levy, {J. M.} and L. Linssen and A. Ljubiĉi{\'c} and J. Long and A. Lupi and A. Marchionni and F. Martelli and X. Mechain and Mendiburu, {J. P.} and Meyer, {J. P.} and M. Mezzetto and Mishra, {S. R.} and Moorhead, {G. F.} and P. Nedelec and Yu 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 J. Rico and P. Riemann and C. Roda and A. Rubbia and F. Salvatore and K. Schahmaneche and B. Schmidt and T. Schmidt and M. Sevior and D. Shih and D. Sillou and Soler, {F. J.P.} and G. Sozzi and D. Steele and U. Stiegler and M. Stipĉevi{\'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 G. Vidal-Sitjes 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",

year = "2003",

month = dec,

day = "11",

doi = "10.1016/j.nima.2003.07.054",

language = "English (US)",

volume = "515",

pages = "800--828",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

number = "3",

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TY - JOUR

T1 - Prediction of neutrino fluxes in the NOMAD experiment

AU - Astier, P.

AU - Autiero, D.

AU - Baldisseri, A.

AU - Baldo-Ceolin, M.

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, S.

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 - Cousins, R.

AU - Daniels, D.

AU - Degaudenzi, H.

AU - Del Prete, T.

AU - de Santo, A.

AU - Dignan, T.

AU - di Lella, L.

AU - do Couto e Silva, E.

AU - Dumarchez, J.

AU - Ellis, M.

AU - Feldman, G. J.

AU - Ferrari, A.

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 - Göbling, C.

AU - Gouanere, M.

AU - Grant, A.

AU - Graziani, G.

AU - Guglielmi, A.

AU - Hagner, C.

AU - Hernando, J.

AU - Hong, T. M.

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 - Lachaud, C.

AU - Lakić, B.

AU - Lanza, A.

AU - la Rotonda, L.

AU - Laveder, M.

AU - Letessier-Selvon, A.

AU - Levy, J. M.

AU - Linssen, L.

AU - Ljubiĉić, A.

AU - Long, J.

AU - Lupi, A.

AU - Marchionni, A.

AU - Martelli, F.

AU - Mechain, X.

AU - Mendiburu, J. P.

AU - Meyer, J. P.

AU - Mezzetto, M.

AU - Mishra, S. R.

AU - Moorhead, G. F.

AU - Nedelec, P.

AU - Nefedov, Yu

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 - Rico, J.

AU - Riemann, P.

AU - Roda, C.

AU - Rubbia, A.

AU - Salvatore, F.

AU - Schahmaneche, K.

AU - Schmidt, B.

AU - Schmidt, T.

AU - Sevior, M.

AU - Shih, D.

AU - Sillou, D.

AU - Soler, F. J.P.

AU - Sozzi, G.

AU - Steele, D.

AU - Stiegler, U.

AU - Stipĉević, 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 - Vidal-Sitjes, G.

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.

PY - 2003/12/11

Y1 - 2003/12/11

N2 - The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for νμ and νe, 10% for ν̄μ, and 12% for ν̄ e. The energy-dependent uncertainty achieved on the ν e/νμ prediction needed for a ν μ→νe oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.

AB - The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for νμ and νe, 10% for ν̄μ, and 12% for ν̄ e. The energy-dependent uncertainty achieved on the ν e/νμ prediction needed for a ν μ→νe oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.

KW - Neutrino beam

KW - Neutrino fluxes

UR - http://www.scopus.com/inward/record.url?scp=0242522303&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0242522303&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2003.07.054

DO - 10.1016/j.nima.2003.07.054

M3 - Article

AN - SCOPUS:0242522303

SN - 0168-9002

VL - 515

SP - 800

EP - 828

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 3

ER -

Prediction of neutrino fluxes in the NOMAD experiment

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