Prediction of Neutrino Fluxes in the NOMAD Experiment

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...

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Detalles Bibliográficos
Autores principales: Astier, P., Autiero, D., Baldisseri, A., Baldo-Ceolin, M., Banner, M., Bassompierre, G., Benslama, K., Besson, N., Bird, I., Blumenfeld, Barry J., Bobisut, F., Bouchez, J., Boyd, S., Bueno, A., Bunyatov, S., Camilleri, L., Cardini, A., Cattaneo, P.W., 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, Malcolm, Feldman, G.J., Ferrari, A., Ferrari, R., Ferrere, D., Flaminio, V., Fraternali, M., Gaillard, J.M., Gangler, E., Geiser, A., Geppert, D., Gibin, D., Gninenko, S., Godley, A., Gomez-Cadenas, J.J., Gosset, J., Gossling, C., Gouanere, M., Grant, A., Graziani, G., Guglielmi, A., Hagner, C., Hernando, J., Hong, T.M., Hubbard, D., Hurst, P., Hyett, N., Iacopini, E., Joseph, C., Juget, F., Kirsanov, M., Klimov, O., Kokkonen, J., Kovzelev, A., Krasnoperov, A., Lachaud, C., Lakic, B., Lanza, A., La Rotonda, L., Laveder, M., Letessier-Selvon, A., Levy, J.M., Linssen, L., Ljubicic, A., Long, J., Lupi, A., Marchionni, A., Martelli, F., Mechain, X., Mendiburu, J.P., Meyer, J.P., Mezzetto, M., Mishra, S.R., Moorhead, G.F., Nedelec, P., Nefedov, Yu., Nguyen-Mau, C., Orestano, D., Pastore, F., Peak, L.S., 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, F.J.P., Sozzi, G., Steele, D., Stiegler, U., Stipcevic, M., Stolarczyk, T., Tareb-Reyes, M., Taylor, G.N., Tereshchenko, V., Toropin, A., Touchard, A.M., Tovey, S.N., Tran, M.T., Tsesmelis, E., Ulrichs, J., Vacavant, L., Valdata-Nappi, M., Valuev, V., Vannucci, F., Varvell, K.E., Veltri, M., Vercesi, V., Vidal-Sitjes, G., Vieira, J.M., Vinogradova, T., Weber, F.V., Weisse, T., Wilson, F.F., Winton, L.J., Yabsley, Bruce D., Zaccone, H., Zuber, K.
Lenguaje:eng
Publicado: 2003
Materias:
Particle Physics - Experiment
Acceso en línea:https://dx.doi.org/10.1016/j.nima.2003.07.054
http://cds.cern.ch/record/620601
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author Astier, P.
Autiero, D.
Baldisseri, A.
Baldo-Ceolin, M.
Banner, M.
Bassompierre, G.
Benslama, K.
Besson, N.
Bird, I.
Blumenfeld, Barry J.
Bobisut, F.
Bouchez, J.
Boyd, S.
Bueno, A.
Bunyatov, S.
Camilleri, L.
Cardini, A.
Cattaneo, P.W.
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, Malcolm
Feldman, G.J.
Ferrari, A.
Ferrari, R.
Ferrere, D.
Flaminio, V.
Fraternali, M.
Gaillard, J.M.
Gangler, E.
Geiser, A.
Geppert, D.
Gibin, D.
Gninenko, S.
Godley, A.
Gomez-Cadenas, J.J.
Gosset, J.
Gossling, C.
Gouanere, M.
Grant, A.
Graziani, G.
Guglielmi, A.
Hagner, C.
Hernando, J.
Hong, T.M.
Hubbard, D.
Hurst, P.
Hyett, N.
Iacopini, E.
Joseph, C.
Juget, F.
Kirsanov, M.
Klimov, O.
Kokkonen, J.
Kovzelev, A.
Krasnoperov, A.
Lachaud, C.
Lakic, B.
Lanza, A.
La Rotonda, L.
Laveder, M.
Letessier-Selvon, A.
Levy, J.M.
Linssen, L.
Ljubicic, A.
Long, J.
Lupi, A.
Marchionni, A.
Martelli, F.
Mechain, X.
Mendiburu, J.P.
Meyer, J.P.
Mezzetto, M.
Mishra, S.R.
Moorhead, G.F.
Nedelec, P.
Nefedov, Yu.
Nguyen-Mau, C.
Orestano, D.
Pastore, F.
Peak, L.S.
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, F.J.P.
Sozzi, G.
Steele, D.
Stiegler, U.
Stipcevic, M.
Stolarczyk, T.
Tareb-Reyes, M.
Taylor, G.N.
Tereshchenko, V.
Toropin, A.
Touchard, A.M.
Tovey, S.N.
Tran, M.T.
Tsesmelis, E.
Ulrichs, J.
Vacavant, L.
Valdata-Nappi, M.
Valuev, V.
Vannucci, F.
Varvell, K.E.
Veltri, M.
Vercesi, V.
Vidal-Sitjes, G.
Vieira, J.M.
Vinogradova, T.
Weber, F.V.
Weisse, T.
Wilson, F.F.
Winton, L.J.
Yabsley, Bruce D.
Zaccone, H.
Zuber, K.
author_facet Astier, P.
Autiero, D.
Baldisseri, A.
Baldo-Ceolin, M.
Banner, M.
Bassompierre, G.
Benslama, K.
Besson, N.
Bird, I.
Blumenfeld, Barry J.
Bobisut, F.
Bouchez, J.
Boyd, S.
Bueno, A.
Bunyatov, S.
Camilleri, L.
Cardini, A.
Cattaneo, P.W.
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, Malcolm
Feldman, G.J.
Ferrari, A.
Ferrari, R.
Ferrere, D.
Flaminio, V.
Fraternali, M.
Gaillard, J.M.
Gangler, E.
Geiser, A.
Geppert, D.
Gibin, D.
Gninenko, S.
Godley, A.
Gomez-Cadenas, J.J.
Gosset, J.
Gossling, C.
Gouanere, M.
Grant, A.
Graziani, G.
Guglielmi, A.
Hagner, C.
Hernando, J.
Hong, T.M.
Hubbard, D.
Hurst, P.
Hyett, N.
Iacopini, E.
Joseph, C.
Juget, F.
Kirsanov, M.
Klimov, O.
Kokkonen, J.
Kovzelev, A.
Krasnoperov, A.
Lachaud, C.
Lakic, B.
Lanza, A.
La Rotonda, L.
Laveder, M.
Letessier-Selvon, A.
Levy, J.M.
Linssen, L.
Ljubicic, A.
Long, J.
Lupi, A.
Marchionni, A.
Martelli, F.
Mechain, X.
Mendiburu, J.P.
Meyer, J.P.
Mezzetto, M.
Mishra, S.R.
Moorhead, G.F.
Nedelec, P.
Nefedov, Yu.
Nguyen-Mau, C.
Orestano, D.
Pastore, F.
Peak, L.S.
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, F.J.P.
Sozzi, G.
Steele, D.
Stiegler, U.
Stipcevic, M.
Stolarczyk, T.
Tareb-Reyes, M.
Taylor, G.N.
Tereshchenko, V.
Toropin, A.
Touchard, A.M.
Tovey, S.N.
Tran, M.T.
Tsesmelis, E.
Ulrichs, J.
Vacavant, L.
Valdata-Nappi, M.
Valuev, V.
Vannucci, F.
Varvell, K.E.
Veltri, M.
Vercesi, V.
Vidal-Sitjes, G.
Vieira, J.M.
Vinogradova, T.
Weber, F.V.
Weisse, T.
Wilson, F.F.
Winton, L.J.
Yabsley, Bruce D.
Zaccone, H.
Zuber, K.
author_sort Astier, P.
collection CERN
description 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 nu(mu) and nu(e), 10% for antinu(mu), and 12% for antinu(e). The energy-dependent uncertainty achieved on the R(e, mu) prediction needed for a nu(mu)->nu(e) oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.
id cern-620601
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
record_format invenio
spelling cern-6206012023-10-24T02:42:50Zdoi:10.1016/j.nima.2003.07.054http://cds.cern.ch/record/620601engAstier, P.Autiero, D.Baldisseri, A.Baldo-Ceolin, M.Banner, M.Bassompierre, G.Benslama, K.Besson, N.Bird, I.Blumenfeld, Barry J.Bobisut, F.Bouchez, J.Boyd, S.Bueno, A.Bunyatov, S.Camilleri, L.Cardini, A.Cattaneo, P.W.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, MalcolmFeldman, G.J.Ferrari, A.Ferrari, R.Ferrere, D.Flaminio, V.Fraternali, M.Gaillard, J.M.Gangler, E.Geiser, A.Geppert, D.Gibin, D.Gninenko, S.Godley, A.Gomez-Cadenas, J.J.Gosset, J.Gossling, C.Gouanere, M.Grant, A.Graziani, G.Guglielmi, A.Hagner, C.Hernando, J.Hong, T.M.Hubbard, D.Hurst, P.Hyett, N.Iacopini, E.Joseph, C.Juget, F.Kirsanov, M.Klimov, O.Kokkonen, J.Kovzelev, A.Krasnoperov, A.Lachaud, C.Lakic, B.Lanza, A.La Rotonda, L.Laveder, M.Letessier-Selvon, A.Levy, J.M.Linssen, L.Ljubicic, A.Long, J.Lupi, A.Marchionni, A.Martelli, F.Mechain, X.Mendiburu, J.P.Meyer, J.P.Mezzetto, M.Mishra, S.R.Moorhead, G.F.Nedelec, P.Nefedov, Yu.Nguyen-Mau, C.Orestano, D.Pastore, F.Peak, L.S.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, F.J.P.Sozzi, G.Steele, D.Stiegler, U.Stipcevic, M.Stolarczyk, T.Tareb-Reyes, M.Taylor, G.N.Tereshchenko, V.Toropin, A.Touchard, A.M.Tovey, S.N.Tran, M.T.Tsesmelis, E.Ulrichs, J.Vacavant, L.Valdata-Nappi, M.Valuev, V.Vannucci, F.Varvell, K.E.Veltri, M.Vercesi, V.Vidal-Sitjes, G.Vieira, J.M.Vinogradova, T.Weber, F.V.Weisse, T.Wilson, F.F.Winton, L.J.Yabsley, Bruce D.Zaccone, H.Zuber, K.Prediction of Neutrino Fluxes in the NOMAD ExperimentParticle Physics - ExperimentThe 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 nu(mu) and nu(e), 10% for antinu(mu), and 12% for antinu(e). The energy-dependent uncertainty achieved on the R(e, mu) prediction needed for a nu(mu)->nu(e) oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.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 nu(mu) and nu(e), 10% for antinu(mu), and 12% for antinu(e). The energy-dependent uncertainty achieved on the R(e, mu) prediction needed for a nu(mu)->nu(e) oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.hep-ex/0306022CERN-EP-2003-032oai:cds.cern.ch:6206012003-06-06
spellingShingle Particle Physics - Experiment
Astier, P.
Autiero, D.
Baldisseri, A.
Baldo-Ceolin, M.
Banner, M.
Bassompierre, G.
Benslama, K.
Besson, N.
Bird, I.
Blumenfeld, Barry J.
Bobisut, F.
Bouchez, J.
Boyd, S.
Bueno, A.
Bunyatov, S.
Camilleri, L.
Cardini, A.
Cattaneo, P.W.
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, Malcolm
Feldman, G.J.
Ferrari, A.
Ferrari, R.
Ferrere, D.
Flaminio, V.
Fraternali, M.
Gaillard, J.M.
Gangler, E.
Geiser, A.
Geppert, D.
Gibin, D.
Gninenko, S.
Godley, A.
Gomez-Cadenas, J.J.
Gosset, J.
Gossling, C.
Gouanere, M.
Grant, A.
Graziani, G.
Guglielmi, A.
Hagner, C.
Hernando, J.
Hong, T.M.
Hubbard, D.
Hurst, P.
Hyett, N.
Iacopini, E.
Joseph, C.
Juget, F.
Kirsanov, M.
Klimov, O.
Kokkonen, J.
Kovzelev, A.
Krasnoperov, A.
Lachaud, C.
Lakic, B.
Lanza, A.
La Rotonda, L.
Laveder, M.
Letessier-Selvon, A.
Levy, J.M.
Linssen, L.
Ljubicic, A.
Long, J.
Lupi, A.
Marchionni, A.
Martelli, F.
Mechain, X.
Mendiburu, J.P.
Meyer, J.P.
Mezzetto, M.
Mishra, S.R.
Moorhead, G.F.
Nedelec, P.
Nefedov, Yu.
Nguyen-Mau, C.
Orestano, D.
Pastore, F.
Peak, L.S.
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, F.J.P.
Sozzi, G.
Steele, D.
Stiegler, U.
Stipcevic, M.
Stolarczyk, T.
Tareb-Reyes, M.
Taylor, G.N.
Tereshchenko, V.
Toropin, A.
Touchard, A.M.
Tovey, S.N.
Tran, M.T.
Tsesmelis, E.
Ulrichs, J.
Vacavant, L.
Valdata-Nappi, M.
Valuev, V.
Vannucci, F.
Varvell, K.E.
Veltri, M.
Vercesi, V.
Vidal-Sitjes, G.
Vieira, J.M.
Vinogradova, T.
Weber, F.V.
Weisse, T.
Wilson, F.F.
Winton, L.J.
Yabsley, Bruce D.
Zaccone, H.
Zuber, K.
Prediction of Neutrino Fluxes in the NOMAD Experiment
title Prediction of Neutrino Fluxes in the NOMAD Experiment
title_full Prediction of Neutrino Fluxes in the NOMAD Experiment
title_fullStr Prediction of Neutrino Fluxes in the NOMAD Experiment
title_full_unstemmed Prediction of Neutrino Fluxes in the NOMAD Experiment
title_short Prediction of Neutrino Fluxes in the NOMAD Experiment
title_sort prediction of neutrino fluxes in the nomad experiment
topic Particle Physics - Experiment
url https://dx.doi.org/10.1016/j.nima.2003.07.054
http://cds.cern.ch/record/620601
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AT lupia predictionofneutrinofluxesinthenomadexperiment
AT marchionnia predictionofneutrinofluxesinthenomadexperiment
AT martellif predictionofneutrinofluxesinthenomadexperiment
AT mechainx predictionofneutrinofluxesinthenomadexperiment
AT mendiburujp predictionofneutrinofluxesinthenomadexperiment
AT meyerjp predictionofneutrinofluxesinthenomadexperiment
AT mezzettom predictionofneutrinofluxesinthenomadexperiment
AT mishrasr predictionofneutrinofluxesinthenomadexperiment
AT moorheadgf predictionofneutrinofluxesinthenomadexperiment
AT nedelecp predictionofneutrinofluxesinthenomadexperiment
AT nefedovyu predictionofneutrinofluxesinthenomadexperiment
AT nguyenmauc predictionofneutrinofluxesinthenomadexperiment
AT orestanod predictionofneutrinofluxesinthenomadexperiment
AT pastoref predictionofneutrinofluxesinthenomadexperiment
AT peakls predictionofneutrinofluxesinthenomadexperiment
AT pennacchioe predictionofneutrinofluxesinthenomadexperiment
AT pessardh predictionofneutrinofluxesinthenomadexperiment
AT pettir predictionofneutrinofluxesinthenomadexperiment
AT placcia predictionofneutrinofluxesinthenomadexperiment
AT polesellog predictionofneutrinofluxesinthenomadexperiment
AT pollmannd predictionofneutrinofluxesinthenomadexperiment
AT polyarusha predictionofneutrinofluxesinthenomadexperiment
AT popovb predictionofneutrinofluxesinthenomadexperiment
AT poulsenc predictionofneutrinofluxesinthenomadexperiment
AT ricoj predictionofneutrinofluxesinthenomadexperiment
AT riemannp predictionofneutrinofluxesinthenomadexperiment
AT rodac predictionofneutrinofluxesinthenomadexperiment
AT rubbiaa predictionofneutrinofluxesinthenomadexperiment
AT salvatoref predictionofneutrinofluxesinthenomadexperiment
AT schahmanechek predictionofneutrinofluxesinthenomadexperiment
AT schmidtb predictionofneutrinofluxesinthenomadexperiment
AT schmidtt predictionofneutrinofluxesinthenomadexperiment
AT seviorm predictionofneutrinofluxesinthenomadexperiment
AT shihd predictionofneutrinofluxesinthenomadexperiment
AT silloud predictionofneutrinofluxesinthenomadexperiment
AT solerfjp predictionofneutrinofluxesinthenomadexperiment
AT sozzig predictionofneutrinofluxesinthenomadexperiment
AT steeled predictionofneutrinofluxesinthenomadexperiment
AT stiegleru predictionofneutrinofluxesinthenomadexperiment
AT stipcevicm predictionofneutrinofluxesinthenomadexperiment
AT stolarczykt predictionofneutrinofluxesinthenomadexperiment
AT tarebreyesm predictionofneutrinofluxesinthenomadexperiment
AT taylorgn predictionofneutrinofluxesinthenomadexperiment
AT tereshchenkov predictionofneutrinofluxesinthenomadexperiment
AT toropina predictionofneutrinofluxesinthenomadexperiment
AT touchardam predictionofneutrinofluxesinthenomadexperiment
AT toveysn predictionofneutrinofluxesinthenomadexperiment
AT tranmt predictionofneutrinofluxesinthenomadexperiment
AT tsesmelise predictionofneutrinofluxesinthenomadexperiment
AT ulrichsj predictionofneutrinofluxesinthenomadexperiment
AT vacavantl predictionofneutrinofluxesinthenomadexperiment
AT valdatanappim predictionofneutrinofluxesinthenomadexperiment
AT valuevv predictionofneutrinofluxesinthenomadexperiment
AT vannuccif predictionofneutrinofluxesinthenomadexperiment
AT varvellke predictionofneutrinofluxesinthenomadexperiment
AT veltrim predictionofneutrinofluxesinthenomadexperiment
AT vercesiv predictionofneutrinofluxesinthenomadexperiment
AT vidalsitjesg predictionofneutrinofluxesinthenomadexperiment
AT vieirajm predictionofneutrinofluxesinthenomadexperiment
AT vinogradovat predictionofneutrinofluxesinthenomadexperiment
AT weberfv predictionofneutrinofluxesinthenomadexperiment
AT weisset predictionofneutrinofluxesinthenomadexperiment
AT wilsonff predictionofneutrinofluxesinthenomadexperiment
AT wintonlj predictionofneutrinofluxesinthenomadexperiment
AT yabsleybruced predictionofneutrinofluxesinthenomadexperiment
AT zacconeh predictionofneutrinofluxesinthenomadexperiment
AT zuberk predictionofneutrinofluxesinthenomadexperiment

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