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High intensity neutrino oscillation facilities in Europe

  • T. R. Edgecock
  • , O. Caretta
  • , T. Davenne
  • , C. Densam
  • , M. Fitton
  • , D. Kelliher
  • , P. Loveridge
  • , S. Machida
  • , C. Prior
  • , C. Rogers
  • , M. Rooney
  • , J. Thomason
  • , D. Wilcox
  • , E. Wildner
  • , I. Efthymiopoulos
  • , R. Garoby
  • , S. Gilardoni
  • , C. Hansen
  • , E. Benedetto
  • , E. Jensen
  • A. Kosmicki, M. Martini, J. Osborne, G. Prior, T. Stora, T. Melo Mendonca, V. Vlachoudis, C. Waaijer, P. Cupial, A. Chancé, A. Longhin, J. Payet, M. Zito, E. Baussan, C. Bobeth, E. Bouquerel, M. Dracos, G. Gaudiot, B. Lepers, F. Osswald, P. Poussot, N. Vassilopoulos, J. Wurtz, V. Zeter, J. Bielski, M. Kozien, L. Lacny, B. Skoczen, B. Szybinski, Aneta Ustrzycka, A. Wroblewski, M. Marie-Jeanne, P. Balint, C. Fourel, J. Giraud, J. Jacob, T. Lamy, L. Latrasse, P. Sortais, T. Thuillier, S. Mitrofanov, M. Loiselet, Th Keutgen, Th Delbar, F. Debray, C. Trophine, S. Veys, C. Daversin, V. Zorin, I. Izotov, V. Skalyga, G. Burt, A. C. Dexter, V. L. Kravchuk, T. Marchi, M. Cinausero, F. Gramegna, G. De Angelis, G. Prete, G. Collazuol, M. Laveder, M. Mazzocco, M. Mezzetto, C. Signorini, E. Vardaci, A. Di Nitto, A. Brondi, G. La Rana, P. Migliozzi, R. Moro, V. Palladino, N. Gelli, D. Berkovits, M. Hass, T. Y. Hirsh, M. Schaumann, A. Stahl, J. Wehner, A. Bross, J. Kopp, D. Neuffer, R. Wands, R. Bayes, A. Laing, P. Soler, S. K. Agarwalla, A. Cervera Villanueva, A. Donini, T. Ghosh, J. J. Gómez Cadenas, P. Hernández, J. Martín-Albo, O. Mena, J. Burguet-Castell, L. Agostino, M. Buizza-Avanzini, M. Marafini, T. Patzak, A. Tonazzo, D. Duchesneau, L. Mosca, M. Bogomilov, Y. Karadzhov, R. Matev, R. Tsenov, E. Akhmedov, M. Blennow, M. Lindner, T. Schwetz, E. Fernández Martinez, M. Maltoni, J. Menéndez, C. Giunti, M. C. González García, J. Salvado, P. Coloma, P. Huber, T. Li, J. López Pavón, C. Orme, S. Pascoli, D. Meloni, J. Tang, W. Winter, T. Ohlsson, H. Zhang, L. Scotto-Lavina, F. Terranova, M. Bonesini, L. Tortora, A. Alekou, M. Aslaninejad, C. Bontoiu, A. Kurup, L. J. Jenner, K. Long, J. Pasternak, J. Pozimski, J. J. Back, P. Harrison, K. Beard, A. Bogacz, J. S. Berg, D. Stratakis, H. Witte, P. Snopok, N. Bliss, M. Cordwell, A. Moss, S. Pattalwar, M. Apollonio
  • STFC Rutherford Appleton Laboratory
  • CERN
  • AGH University of Krakow
  • Centre d'Etudes de Saclay
  • Université de Strasbourg
  • Cracow University of Technology
  • Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
  • Université catholique de Louvain
  • Lab. Natl. Champs Magnetiques Pulses
  • Institute of Applied Physics of the Russian Academy of Sciences
  • Lancaster University
  • Laboratori Nazionali di Legnaro
  • University of Padua
  • National Institute for Nuclear Physics
  • Weizmann Institute of Science
  • RWTH Aachen University
  • Fermi National Accelerator Laboratory
  • University of Glasgow
  • University of Valencia
  • Universitat de Illes Balears
  • PSL University
  • Université Savoie Mont Blanc
  • Laboratoire Souterrain de Modane
  • Sofia University St. Kliment Ohridski
  • Max Planck Institute for Nuclear Physics
  • Universidad Autónoma de Madrid
  • University of Barcelona
  • Virginia Polytechnic Institute and State University
  • Durham University
  • University of Würzburg
  • AlbaNova University Center
  • University of Zurich
  • Imperial College London
  • University of Warwick
  • Muons, Inc.
  • Thomas Jefferson National Accelerator Facility
  • Brookhaven National Laboratory
  • Illinois Institute of Technology
  • Daresbury Laboratory
  • Diamond Light Source

Research output: Contribution to journalArticlepeer-review

53 Scopus citations

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 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.

Original languageEnglish
Article number021002
JournalPhysical Review Special Topics - Accelerators and Beams
Volume16
Issue number2
DOIs
StatePublished - Feb 20 2013

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