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High intensity neutrino oscillation facilities in Europe

The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Pr...

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Detalles Bibliográficos
Autores principales: Edgecock, T.R., Caretta, O., Davenne, T., Densham, C., Fitton, M., Kelliher, D., Loveridge, P., Machida, S., Prior, C., Rogers, C., Rooney, M., Thomason, J., Wilcox, D., Wildner, E., Efthymiopoulos, I., Garoby, R., Gilardoni, S., Hansen, C., Benedetto, E., Jensen, E., Kosmicki, A., Martini, M., Osborne, J., Prior, G., Stora, T., Melo-Mendonca, T., Vlachoudis, V., Waaijer, C., Cupial, P., Chancé, A., Longhin, A., Payet, J., Zito, M., Baussan, E., Bobeth, C., Bouquerel, E., Dracos, M., Gaudiot, G., Lepers, B., Osswald, F., Poussot, P., Vassilopoulos, N., Wurtz, J., Zeter, V., Bielski, J., Kozien, M., Lacny, L., Skoczen, B., Szybinski, B., Ustrzycka, A., Wroblewski, A., Marie-Jeanne, M., Balint, P., Fourel, C., Giraud, J., Jacob, J., Lamy, T., Latrasse, L., Sortais, P., Thuillier, T., Mitrofanov, S., Loiselet, M., Keutgen, Th., Delbar, Th., Debray, F., Trophine, C., Veys, S., Daversin, C., Zorin, V., Izotov, I., Skalyga, V., Burt, G., Dexter, A.C., Kravchuk, V.L., Marchi, T., Cinausero, M., Gramegna, F., De Angelis, G., Prete, G., Collazuol, G., Laveder, M., Mazzocco, M., Mezzetto, M., Signorini, C., Vardaci, E., Di Nitto, A., Brondi, A., La Rana, G., Migliozzi, P., Moro, R., Palladino, V., Gelli, N., Berkovits, D., Hass, M., Hirsh, T.Y., Schaumann, M., Stahl, A., Wehner, J., Bross, A., Kopp, J., Neuffer, D., Wands, R., Bayes, R., Laing, A., Soler, P., Agarwalla, S.K., Cervera Villanueva, A., Donini, A., Ghosh, T., Gómez Cadenas, J.J., Hernández, P., Martín-Albo, J., Mena, O., Burguet-Castell, J., Agostino, L., Buizza-Avanzini, M., Marafini, M., Patzak, T., Tonazzo, A., Duchesneau, D., Mosca, L., Bogomilov, M., Karadzhov, Y., Matev, R., Tsenov, R., Akhmedov, E., Blennow, M., Lindner, M., Schwetz, T., Fernández Martinez, E., Maltoni, M., Menéndez, J., Giunti, C., González García, M. C., Salvado, J., Coloma, P., Huber, P., Li, T., López-Pavón, J., Orme, C., Pascoli, S., Meloni, D., Tang, J., Winter, W., Ohlsson, T., Zhang, H., Scotto-Lavina, L., Terranova, F., Bonesini, M., Tortora, L., Alekou, A., Aslaninejad, M., Bontoiu, C., Kurup, A., Jenner, L.J., Long, K., Pasternak, J., Pozimski, J., Back, J.J., Harrison, P., Beard, K., Bogacz, A., Berg, J.S., Stratakis, D., Witte, H., Snopok, P., Bliss, N., Cordwell, M., Moss, A., Pattalwar, S., Apollonio, M.
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevSTAB.16.021002
https://dx.doi.org/10.1103/PhysRevAccelBeams.19.079901
http://cds.cern.ch/record/1548053
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author Edgecock, T.R.
Caretta, O.
Davenne, T.
Densham, C.
Fitton, M.
Kelliher, D.
Loveridge, P.
Machida, S.
Prior, C.
Rogers, C.
Rooney, M.
Thomason, J.
Wilcox, D.
Wildner, E.
Efthymiopoulos, I.
Garoby, R.
Gilardoni, S.
Hansen, C.
Benedetto, E.
Jensen, E.
Kosmicki, A.
Martini, M.
Osborne, J.
Prior, G.
Stora, T.
Melo-Mendonca, T.
Vlachoudis, V.
Waaijer, C.
Cupial, P.
Chancé, A.
Longhin, A.
Payet, J.
Zito, M.
Baussan, E.
Bobeth, C.
Bouquerel, E.
Dracos, M.
Gaudiot, G.
Lepers, B.
Osswald, F.
Poussot, P.
Vassilopoulos, N.
Wurtz, J.
Zeter, V.
Bielski, J.
Kozien, M.
Lacny, L.
Skoczen, B.
Szybinski, B.
Ustrzycka, A.
Wroblewski, A.
Marie-Jeanne, M.
Balint, P.
Fourel, C.
Giraud, J.
Jacob, J.
Lamy, T.
Latrasse, L.
Sortais, P.
Thuillier, T.
Mitrofanov, S.
Loiselet, M.
Keutgen, Th.
Delbar, Th.
Debray, F.
Trophine, C.
Veys, S.
Daversin, C.
Zorin, V.
Izotov, I.
Skalyga, V.
Burt, G.
Dexter, A.C.
Kravchuk, V.L.
Marchi, T.
Cinausero, M.
Gramegna, F.
De Angelis, G.
Prete, G.
Collazuol, G.
Laveder, M.
Mazzocco, M.
Mezzetto, M.
Signorini, C.
Vardaci, E.
Di Nitto, A.
Brondi, A.
La Rana, G.
Migliozzi, P.
Moro, R.
Palladino, V.
Gelli, N.
Berkovits, D.
Hass, M.
Hirsh, T.Y.
Schaumann, M.
Stahl, A.
Wehner, J.
Bross, A.
Kopp, J.
Neuffer, D.
Wands, R.
Bayes, R.
Laing, A.
Soler, P.
Agarwalla, S.K.
Cervera Villanueva, A.
Donini, A.
Ghosh, T.
Gómez Cadenas, J.J.
Hernández, P.
Martín-Albo, J.
Mena, O.
Burguet-Castell, J.
Agostino, L.
Buizza-Avanzini, M.
Marafini, M.
Patzak, T.
Tonazzo, A.
Duchesneau, D.
Mosca, L.
Bogomilov, M.
Karadzhov, Y.
Matev, R.
Tsenov, R.
Akhmedov, E.
Blennow, M.
Lindner, M.
Schwetz, T.
Fernández Martinez, E.
Maltoni, M.
Menéndez, J.
Giunti, C.
González García, M. C.
Salvado, J.
Coloma, P.
Huber, P.
Li, T.
López-Pavón, J.
Orme, C.
Pascoli, S.
Meloni, D.
Tang, J.
Winter, W.
Ohlsson, T.
Zhang, H.
Scotto-Lavina, L.
Terranova, F.
Bonesini, M.
Tortora, L.
Alekou, A.
Aslaninejad, M.
Bontoiu, C.
Kurup, A.
Jenner, L.J.
Long, K.
Pasternak, J.
Pozimski, J.
Back, J.J.
Harrison, P.
Beard, K.
Bogacz, A.
Berg, J.S.
Stratakis, D.
Witte, H.
Snopok, P.
Bliss, N.
Cordwell, M.
Moss, A.
Pattalwar, S.
Apollonio, M.
author_facet Edgecock, T.R.
Caretta, O.
Davenne, T.
Densham, C.
Fitton, M.
Kelliher, D.
Loveridge, P.
Machida, S.
Prior, C.
Rogers, C.
Rooney, M.
Thomason, J.
Wilcox, D.
Wildner, E.
Efthymiopoulos, I.
Garoby, R.
Gilardoni, S.
Hansen, C.
Benedetto, E.
Jensen, E.
Kosmicki, A.
Martini, M.
Osborne, J.
Prior, G.
Stora, T.
Melo-Mendonca, T.
Vlachoudis, V.
Waaijer, C.
Cupial, P.
Chancé, A.
Longhin, A.
Payet, J.
Zito, M.
Baussan, E.
Bobeth, C.
Bouquerel, E.
Dracos, M.
Gaudiot, G.
Lepers, B.
Osswald, F.
Poussot, P.
Vassilopoulos, N.
Wurtz, J.
Zeter, V.
Bielski, J.
Kozien, M.
Lacny, L.
Skoczen, B.
Szybinski, B.
Ustrzycka, A.
Wroblewski, A.
Marie-Jeanne, M.
Balint, P.
Fourel, C.
Giraud, J.
Jacob, J.
Lamy, T.
Latrasse, L.
Sortais, P.
Thuillier, T.
Mitrofanov, S.
Loiselet, M.
Keutgen, Th.
Delbar, Th.
Debray, F.
Trophine, C.
Veys, S.
Daversin, C.
Zorin, V.
Izotov, I.
Skalyga, V.
Burt, G.
Dexter, A.C.
Kravchuk, V.L.
Marchi, T.
Cinausero, M.
Gramegna, F.
De Angelis, G.
Prete, G.
Collazuol, G.
Laveder, M.
Mazzocco, M.
Mezzetto, M.
Signorini, C.
Vardaci, E.
Di Nitto, A.
Brondi, A.
La Rana, G.
Migliozzi, P.
Moro, R.
Palladino, V.
Gelli, N.
Berkovits, D.
Hass, M.
Hirsh, T.Y.
Schaumann, M.
Stahl, A.
Wehner, J.
Bross, A.
Kopp, J.
Neuffer, D.
Wands, R.
Bayes, R.
Laing, A.
Soler, P.
Agarwalla, S.K.
Cervera Villanueva, A.
Donini, A.
Ghosh, T.
Gómez Cadenas, J.J.
Hernández, P.
Martín-Albo, J.
Mena, O.
Burguet-Castell, J.
Agostino, L.
Buizza-Avanzini, M.
Marafini, M.
Patzak, T.
Tonazzo, A.
Duchesneau, D.
Mosca, L.
Bogomilov, M.
Karadzhov, Y.
Matev, R.
Tsenov, R.
Akhmedov, E.
Blennow, M.
Lindner, M.
Schwetz, T.
Fernández Martinez, E.
Maltoni, M.
Menéndez, J.
Giunti, C.
González García, M. C.
Salvado, J.
Coloma, P.
Huber, P.
Li, T.
López-Pavón, J.
Orme, C.
Pascoli, S.
Meloni, D.
Tang, J.
Winter, W.
Ohlsson, T.
Zhang, H.
Scotto-Lavina, L.
Terranova, F.
Bonesini, M.
Tortora, L.
Alekou, A.
Aslaninejad, M.
Bontoiu, C.
Kurup, A.
Jenner, L.J.
Long, K.
Pasternak, J.
Pozimski, J.
Back, J.J.
Harrison, P.
Beard, K.
Bogacz, A.
Berg, J.S.
Stratakis, D.
Witte, H.
Snopok, P.
Bliss, N.
Cordwell, M.
Moss, A.
Pattalwar, S.
Apollonio, M.
author_sort Edgecock, T.R.
collection CERN
description The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Fr\'ejus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of {\mu}+ and {\mu}- beams in a storage ring. The far detector in this case is a 100 kt Magnetised Iron Neutrino Detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neutrinos come from the decay of beta emitting isotopes, in particular 6He and 18Ne, also stored in a ring. The far detector is also the MEMPHYS detector in the Fr\'ejus tunnel. EUROnu has undertaken conceptual designs of these facilities and studied the performance of the detectors. Based on this, it has determined the physics reach of each facility, in particular for the measurement of CP violation in the lepton sector, and estimated the cost of construction. These have demonstrated that the best facility to build is the Neutrino Factory. However, if a powerful proton driver is constructed for another purpose or if the MEMPHYS detector is built for astroparticle physics, the Super Beam also becomes very attractive.
id cern-1548053
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
record_format invenio
spelling cern-15480532022-03-30T02:03:22Zdoi:10.1103/PhysRevSTAB.16.021002doi:10.1103/PhysRevAccelBeams.19.079901http://cds.cern.ch/record/1548053engEdgecock, T.R.Caretta, O.Davenne, T.Densham, C.Fitton, M.Kelliher, D.Loveridge, P.Machida, S.Prior, C.Rogers, C.Rooney, M.Thomason, J.Wilcox, D.Wildner, E.Efthymiopoulos, I.Garoby, R.Gilardoni, S.Hansen, C.Benedetto, E.Jensen, E.Kosmicki, A.Martini, M.Osborne, J.Prior, G.Stora, T.Melo-Mendonca, T.Vlachoudis, V.Waaijer, C.Cupial, P.Chancé, A.Longhin, A.Payet, J.Zito, M.Baussan, E.Bobeth, C.Bouquerel, E.Dracos, M.Gaudiot, G.Lepers, B.Osswald, F.Poussot, P.Vassilopoulos, N.Wurtz, J.Zeter, V.Bielski, J.Kozien, M.Lacny, L.Skoczen, B.Szybinski, B.Ustrzycka, A.Wroblewski, A.Marie-Jeanne, M.Balint, P.Fourel, C.Giraud, J.Jacob, J.Lamy, T.Latrasse, L.Sortais, P.Thuillier, T.Mitrofanov, S.Loiselet, M.Keutgen, Th.Delbar, Th.Debray, F.Trophine, C.Veys, S.Daversin, C.Zorin, V.Izotov, I.Skalyga, V.Burt, G.Dexter, A.C.Kravchuk, V.L.Marchi, T.Cinausero, M.Gramegna, F.De Angelis, G.Prete, G.Collazuol, G.Laveder, M.Mazzocco, M.Mezzetto, M.Signorini, C.Vardaci, E.Di Nitto, A.Brondi, A.La Rana, G.Migliozzi, P.Moro, R.Palladino, V.Gelli, N.Berkovits, D.Hass, M.Hirsh, T.Y.Schaumann, M.Stahl, A.Wehner, J.Bross, A.Kopp, J.Neuffer, D.Wands, R.Bayes, R.Laing, A.Soler, P.Agarwalla, S.K.Cervera Villanueva, A.Donini, A.Ghosh, T.Gómez Cadenas, J.J.Hernández, P.Martín-Albo, J.Mena, O.Burguet-Castell, J.Agostino, L.Buizza-Avanzini, M.Marafini, M.Patzak, T.Tonazzo, A.Duchesneau, D.Mosca, L.Bogomilov, M.Karadzhov, Y.Matev, R.Tsenov, R.Akhmedov, E.Blennow, M.Lindner, M.Schwetz, T.Fernández Martinez, E.Maltoni, M.Menéndez, J.Giunti, C.González García, M. C.Salvado, J.Coloma, P.Huber, P.Li, T.López-Pavón, J.Orme, C.Pascoli, S.Meloni, D.Tang, J.Winter, W.Ohlsson, T.Zhang, H.Scotto-Lavina, L.Terranova, F.Bonesini, M.Tortora, L.Alekou, A.Aslaninejad, M.Bontoiu, C.Kurup, A.Jenner, L.J.Long, K.Pasternak, J.Pozimski, J.Back, J.J.Harrison, P.Beard, K.Bogacz, A.Berg, J.S.Stratakis, D.Witte, H.Snopok, P.Bliss, N.Cordwell, M.Moss, A.Pattalwar, S.Apollonio, M.High intensity neutrino oscillation facilities in EuropeAccelerators and Storage RingsThe EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Fr\'ejus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of {\mu}+ and {\mu}- beams in a storage ring. The far detector in this case is a 100 kt Magnetised Iron Neutrino Detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neutrinos come from the decay of beta emitting isotopes, in particular 6He and 18Ne, also stored in a ring. The far detector is also the MEMPHYS detector in the Fr\'ejus tunnel. EUROnu has undertaken conceptual designs of these facilities and studied the performance of the detectors. Based on this, it has determined the physics reach of each facility, in particular for the measurement of CP violation in the lepton sector, and estimated the cost of construction. These have demonstrated that the best facility to build is the Neutrino Factory. However, if a powerful proton driver is constructed for another purpose or if the MEMPHYS detector is built for astroparticle physics, the Super Beam also becomes very attractive.The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Fréjus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of μ+ and μ- beams in a storage ring. The far detector in this case is a 100 kt magnetized iron neutrino detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neutrinos come from the decay of beta emitting isotopes, in particular He6 and Ne18, also stored in a ring. The far detector is also the MEMPHYS detector in the Fréjus tunnel. EUROnu has undertaken conceptual designs of these facilities and studied the performance of the detectors. Based on this, it has determined the physics reach of each facility, in particular for the measurement of CP violation in the lepton sector, and estimated the cost of construction. These have demonstrated that the best facility to build is the Neutrino Factory. However, if a powerful proton driver is constructed for another purpose or if the MEMPHYS detector is built for astroparticle physics, the Super Beam also becomes very attractive.The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Fr\'ejus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of {\mu}+ and {\mu}- beams in a storage ring. The far detector in this case is a 100 kt Magnetised Iron Neutrino Detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neutrinos come from the decay of beta emitting isotopes, in particular 6He and 18Ne, also stored in a ring. The far detector is also the MEMPHYS detector in the Fr\'ejus tunnel. EUROnu has undertaken conceptual designs of these facilities and studied the performance of the detectors. Based on this, it has determined the physics reach of each facility, in particular for the measurement of CP violation in the lepton sector, and estimated the cost of construction. These have demonstrated that the best facility to build is the Neutrino Factory. However, if a powerful proton driver is constructed for another purpose or if the MEMPHYS detector is built for astroparticle physics, the Super Beam also becomes very attractive.arXiv:1305.4067FERMILAB-PUB-13-656-APC-PPDoai:cds.cern.ch:15480532013-05-17
spellingShingle Accelerators and Storage Rings
Edgecock, T.R.
Caretta, O.
Davenne, T.
Densham, C.
Fitton, M.
Kelliher, D.
Loveridge, P.
Machida, S.
Prior, C.
Rogers, C.
Rooney, M.
Thomason, J.
Wilcox, D.
Wildner, E.
Efthymiopoulos, I.
Garoby, R.
Gilardoni, S.
Hansen, C.
Benedetto, E.
Jensen, E.
Kosmicki, A.
Martini, M.
Osborne, J.
Prior, G.
Stora, T.
Melo-Mendonca, T.
Vlachoudis, V.
Waaijer, C.
Cupial, P.
Chancé, A.
Longhin, A.
Payet, J.
Zito, M.
Baussan, E.
Bobeth, C.
Bouquerel, E.
Dracos, M.
Gaudiot, G.
Lepers, B.
Osswald, F.
Poussot, P.
Vassilopoulos, N.
Wurtz, J.
Zeter, V.
Bielski, J.
Kozien, M.
Lacny, L.
Skoczen, B.
Szybinski, B.
Ustrzycka, A.
Wroblewski, A.
Marie-Jeanne, M.
Balint, P.
Fourel, C.
Giraud, J.
Jacob, J.
Lamy, T.
Latrasse, L.
Sortais, P.
Thuillier, T.
Mitrofanov, S.
Loiselet, M.
Keutgen, Th.
Delbar, Th.
Debray, F.
Trophine, C.
Veys, S.
Daversin, C.
Zorin, V.
Izotov, I.
Skalyga, V.
Burt, G.
Dexter, A.C.
Kravchuk, V.L.
Marchi, T.
Cinausero, M.
Gramegna, F.
De Angelis, G.
Prete, G.
Collazuol, G.
Laveder, M.
Mazzocco, M.
Mezzetto, M.
Signorini, C.
Vardaci, E.
Di Nitto, A.
Brondi, A.
La Rana, G.
Migliozzi, P.
Moro, R.
Palladino, V.
Gelli, N.
Berkovits, D.
Hass, M.
Hirsh, T.Y.
Schaumann, M.
Stahl, A.
Wehner, J.
Bross, A.
Kopp, J.
Neuffer, D.
Wands, R.
Bayes, R.
Laing, A.
Soler, P.
Agarwalla, S.K.
Cervera Villanueva, A.
Donini, A.
Ghosh, T.
Gómez Cadenas, J.J.
Hernández, P.
Martín-Albo, J.
Mena, O.
Burguet-Castell, J.
Agostino, L.
Buizza-Avanzini, M.
Marafini, M.
Patzak, T.
Tonazzo, A.
Duchesneau, D.
Mosca, L.
Bogomilov, M.
Karadzhov, Y.
Matev, R.
Tsenov, R.
Akhmedov, E.
Blennow, M.
Lindner, M.
Schwetz, T.
Fernández Martinez, E.
Maltoni, M.
Menéndez, J.
Giunti, C.
González García, M. C.
Salvado, J.
Coloma, P.
Huber, P.
Li, T.
López-Pavón, J.
Orme, C.
Pascoli, S.
Meloni, D.
Tang, J.
Winter, W.
Ohlsson, T.
Zhang, H.
Scotto-Lavina, L.
Terranova, F.
Bonesini, M.
Tortora, L.
Alekou, A.
Aslaninejad, M.
Bontoiu, C.
Kurup, A.
Jenner, L.J.
Long, K.
Pasternak, J.
Pozimski, J.
Back, J.J.
Harrison, P.
Beard, K.
Bogacz, A.
Berg, J.S.
Stratakis, D.
Witte, H.
Snopok, P.
Bliss, N.
Cordwell, M.
Moss, A.
Pattalwar, S.
Apollonio, M.
High intensity neutrino oscillation facilities in Europe
title High intensity neutrino oscillation facilities in Europe
title_full High intensity neutrino oscillation facilities in Europe
title_fullStr High intensity neutrino oscillation facilities in Europe
title_full_unstemmed High intensity neutrino oscillation facilities in Europe
title_short High intensity neutrino oscillation facilities in Europe
title_sort high intensity neutrino oscillation facilities in europe
topic Accelerators and Storage Rings
url https://dx.doi.org/10.1103/PhysRevSTAB.16.021002
https://dx.doi.org/10.1103/PhysRevAccelBeams.19.079901
http://cds.cern.ch/record/1548053
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