학술논문

The EUROnu Project
Document Type
Working Paper
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.Ustrycka, 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.Villanueva, A. CerveraDonini, A.Ghosh, T.Cadenas, J. J. GómezHernández, 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.Martinez, E. FernándezMaltoni, M.Menéndez, J.Giunti, C.García, M. C. GonzálezSalvado, 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.
Source
Phys. Rev. ST Accel. Beams 16 021002 (2013)
Subject
Physics - Accelerator Physics
High Energy Physics - Experiment
Language
Abstract
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.
Comment: Results from the Framework Programme 7 project EUROnu, which studied three possible accelerator facilities for future high intensity neutrino oscillation facilities in Europe