SOX: Short Distance Neutrino Oscillations with Borexino

Bravo-Berguno, D.; Agostini, M.; Althenmuller, K.; Bellini, G.; Benziger, J.; Berton, N.; Bick, D.; Bonfini, G.; Caccianiga, B.; Cadonati, L.; Calaprice, F.; Caminata, A.; Cavalcante, P.; Chavarria, A.; Chepurnov, A.; Cribier, M.; D'Angelo, D.; Davini, S.; Derbin, A.; di Noto, L.; Durero, M.; Empl, A.; Etenko, A.; Farinon, S.; Fischer, V.; Fomenko, K.; Franco, D.; Gabriele, F.; Gaffiot, J.; Galbiati, C.; Gazzana, S.; Ghiano, C.; Giammarchi, M.; Goger-Neff, M.; Goretti, A.; Grandi, L.; Gromov, M.; Hagner, C.; Houdy,; Hungerford, E.; Ianni, A.; Ianni, A.; Jonqueres, N.; Kobychev, V.; Korablev, D.; Korga, G.; Kryn, D.; Lasserre, T.; Laubenstein, M.; Lehnert, B.; Lewke, T.; Link, J.; Litvinovich, E.; Lombardi, F.; Lombardi, P.; Ludhova, L.; Lukyanchenko, G.; Machulin, I.; Manecki, S.; Maneschg, W.; Marcocci, S.; Maricic, J.; Meindl, Q.; Mention, G.; Meroni, E.; Meyer, M.; Miramonti, L.; Misiaszek, M.; Montuschi, M.; Mosteiro, P.; Muratova, V.; Musenich, R.; Oberauer, L.; Obolensky, M.; Ortica,; Otis, K.; Pallavicini, M.; Papp, L.; Perasso, L.; Pocar, A.; Ranucci, G.; Razeto, A.; Re, A.; Romani, A.; Rossi, N.; Saldanha, R.; Salvo, C.; Schonert, S.; Scola, L.; Simgen, H.; Skorokhvatov, M.; Smirnov, O.; Sotnikov, A.; Sukhotin, S.; Suvorov, Y.; Tartagli, R.; Testera, G.; Veyssiere, C.; Vivier, M.; Vogelaar, R. B.; von Feilitzsch, F.; Wang, H.; Winter, J.; Wojcik, M.; Wright, A.; Wurm, M.; Zaimidorogan, O.; Zavatarelli, S.; Zuber, K.; Zuzel, G.

doi:10.1016/j.nuclphysbps.2015.09.283

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 ν e (Cr) and ν e (Ce). Interacting in the active volume of the liquid scintillator, each beam would create a spatial wave pattern in case of oscillation of the ν e (or ν e ) 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.

SOX: Short Distance Neutrino Oscillations with Borexino

Bravo-Berguno D.;Agostini M.;Althenmuller K.;Bellini G.;Benziger J.;Berton N.;Bick D.;Bonfini G.;Caccianiga B.;Cadonati L.;Calaprice F.;Caminata A.;Cavalcante P.;Chavarria A.;Chepurnov A.;Cribier M.;D'Angelo D.;Davini S.;Derbin A.;di Noto L.;Durero M.;Empl A.;Etenko A.;Farinon S.;Fischer V.;Fomenko K.;Franco D.;Gabriele F.;Gaffiot J.;Galbiati C.;Gazzana S.;Ghiano C.;Giammarchi M.;Goger-Neff M.;Goretti A.;Grandi L.;Gromov M.;Hagner C.;Houdy;Hungerford E.;Ianni A.;Ianni A.;Jonqueres N.;Kobychev V.;Korablev D.;Korga G.;Kryn D.;Lasserre T.;Laubenstein M.;Lehnert B.;Lewke T.;Link J.;Litvinovich E.;Lombardi F.;Lombardi P.;Ludhova L.;Lukyanchenko G.;Machulin I.;Manecki S.;Maneschg W.;Marcocci S.;Maricic J.;Meindl Q.;Mention G.;Meroni E.;Meyer M.;Miramonti L.;Misiaszek M.;Montuschi M.;Mosteiro P.;Muratova V.;Musenich R.;Oberauer L.;Obolensky M.;Ortica;Otis K.;Pallavicini M.;Papp L.;Perasso L.;Pocar A.;Ranucci G.;Razeto A.;Re A.;Romani A.;Rossi N.;Saldanha R.;Salvo C.;Schonert S.;Scola L.;Simgen H.;Skorokhvatov M.;Smirnov O.;Sotnikov A.;Sukhotin S.;Suvorov Y.;Tartagli R.;Testera G.;Veyssiere C.;Vivier M.;Vogelaar R. B.;von Feilitzsch F.;Wang H.;Winter J.;Wojcik M.;Wright A.;Wurm M.;Zaimidorogan O.;Zavatarelli S.;Zuber K.;Zuzel G.

2016-01-01

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 ν e (Cr) and ν e (Ce). Interacting in the active volume of the liquid scintillator, each beam would create a spatial wave pattern in case of oscillation of the ν e (or ν e ) 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.