/ Experiment-HEP

SOX: Short Distance Neutrino Oscillations with Borexino

Bravo-Berguño, D. (Virginia Tech.) ; Agostini, M. (Munich, Tech. U.) ; Althenmüller, K. (Munich, Tech. U.) ; Bellini, G. (INFN, Milan) ; Benziger, J. (Princeton U.) ; Berton, N. (IRFU, SPhN, Saclay) ; Bick, D. (Hamburg U.) ; Bonfini, G. (Gran Sasso) ; Caccianiga, B. (INFN, Milan) ; Cadonati, L. (Massachusetts U., Amherst) ; Calaprice, F. (Princeton U.) ; Caminata, A. (INFN, Genoa) ; Cavalcante, P. (Gran Sasso) ; Chavarria, A. (Princeton U.) ; Chepurnov, A. (SINP, Moscow) ; Cribier, M. (APC, Paris) ; D'Angelo, D. (INFN, Milan) ; Davini, S. (Houston U.) ; Derbin, A. (St. Petersburg, INP) ; di Noto, L. (INFN, Genoa) ; Durero, M. (IRFU, SPhN, Saclay) ; Empl, A. (Houston U.) ; Etenko, A. (Moscow Phys. Eng. Inst.) ; Farinon, S. (INFN, Genoa) ; Fischer, V. (IRFU, SPhN, Saclay) ; Fomenko, K. (Dubna, JINR) ; Franco, D. (APC, Paris) ; Gabriele, F. (Gran Sasso) ; Gaffiot, J. (Moscow, KSRS) ; Galbiati, C. (Princeton U.) ; Gazzana, S. (Moscow, KSRS) ; Ghiano, C. (INFN, Genoa) ; Giammarchi, M. (INFN, Milan) ; Göger-Neff, M. (Munich, Tech. U.) ; Goretti, A. (Gran Sasso) ; Grandi, L. (INFN, Genoa) ; Gromov, M. (SINP, Moscow) ; Hagner, C. (Hamburg U.) ; Houdy, Th. (APC, Paris) ; Hungerford, E. (Houston U.) ; Ianni, Aldo (Moscow, KSRS) ; Ianni, Andrea (Princeton U.) ; Jonquères, N. (IRFU, SPhN, Saclay) ; Kobychev, V. (Kiev, INR) ; Korablev, D. (Dubna, JINR) ; Korga, G. (Houston U.) ; Kryn, D. (APC, Paris) ; Lasserre, T. (IRFU, SPhN, Saclay) ; Laubenstein, M. (Moscow, KSRS) ; Lehnert, B. (Munich, Tech. U.) ; Lewke, T. (Munich, Tech. U.) ; Link, J. (Virginia Tech.) ; Litvinovich, E. (Moscow Phys. Eng. Inst.) ; Lombardi, F. (Moscow, KSRS) ; Lombardi, P. (INFN, Milan) ; Ludhova, L. (INFN, Milan) ; Lukyanchenko, G. (Moscow, KSRS) ; Machulin, I. (Moscow Phys. Eng. Inst.) ; Manecki, S. (Virginia Tech.) ; Maneschg, W. (Heidelberg, Max Planck Inst.) ; Marcocci, S. (Gran Sasso) ; Maricic, J. (Hawaii U.) ; Meindl, Q. (Munich, Tech. U.) ; Mention, G. (IRFU, SPhN, Saclay) ; Meroni, E. (INFN, Milan) ; Meyer, M. (Hamburg U.) ; Miramonti, L. (INFN, Milan) ; Misiaszek, M. (Jagiellonian U.) ; Montuschi, M. (Moscow, KSRS) ; Mosteiro, P. (Princeton U.) ; Muratova, V. (St. Petersburg, INP) ; Musenich, R. (INFN, Genoa) ; Oberauer, L. (Munich, Tech. U.) ; Obolensky, M. (APC, Paris) ; Ortica, F. (Perugia U.) ; Otis, K. (Massachusetts U., Amherst) ; Pallavicini, M. (INFN, Genoa) ; Papp, L. (Munich, Tech. U.) ; Perasso, L. (INFN, Genoa) ; Pocar, A. (Massachusetts U., Amherst) ; Ranucci, G. (INFN, Milan) ; Razeto, A. (Moscow, KSRS) ; Re, A. (INFN, Milan) ; Romani, A. (Perugia U.) ; Rossi, N. (Moscow, KSRS) ; Saldanha, R. (Princeton U.) ; Salvo, C. (INFN, Genoa) ; Schönert, S. (Munich, Tech. U.) ; Scola, L. (IRFU, SPhN, Saclay) ; Simgen, H. (Heidelberg, Max Planck Inst.) ; Skorokhvatov, M. (Moscow Phys. Eng. Inst.) ; Smirnov, O. (Dubna, JINR) ; Sotnikov, A. (Dubna, JINR) ; Sukhotin, S. (Moscow Phys. Eng. Inst.) ; Suvorov, Y. (Perugia U.) ; Tartaglia, R. (Moscow, KSRS) ; Testera, G. (INFN, Genoa) ; Veyssière, C. (IRFU, SPhN, Saclay) ; Vivier, M. (IRFU, SPhN, Saclay) ; Vogelaar, R.B. (Virginia Tech.) ; von Feilitzsch, F. (Munich, Tech. U.) ; Wang, H. (UCLA) ; Winter, J. (Munich, Tech. U.) ; Wojcik, M. (Jagiellonian U.) ; Wright, A. (Princeton U.) ; Wurm, M. (Mainz U., Inst. Phys.) ; Zaimidoroga, O. (Dubna, JINR) ; Zavatarelli, S. (INFN, Genoa) ; Zuber, K. (Dresden, Tech. U., ITP) ; Zuzel, G. (Jagiellonian U.)

Published in: Nucl.Part.Phys.Proc.
Year: 2016
Vol.: 273-275
Page No: 1760-1764
Pages: 5
Year: 2016-06-02

Abstract: The Borexino detector has convincingly shown its outstanding performance in the in the sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection, which make it the ideal tool to unambiguously test the long-standing issue of the existence of a sterile neutrino, as suggested by several anomalies: the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar ν experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on chromium and cerium, which deployed under the experiment will emit two intense beams of νe (Cr) and νe‾ (Ce). Interacting in the active volume of the liquid scintillator, each beam would create a spatial wave pattern in case of oscillation of the νe (or νe‾ ) into the sterile state, which would be the smoking gun proving the existence of the new sterile member of the neutrino family. Otherwise, its absence will allow setting very stringent limit on its existence.

Keyword(s): SOX ; sterile neutrinos ; anomalous oscillations ; chromium-51 ; cerium-144 ; Borexino

Total numbers of views: 393
Numbers of unique views: 227
DOI: 10.1016/j.nuclphysbps.2015.09.283
 Record created 2016-07-04, last modified 2016-07-04

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