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Short distance neutrino oscillations with Borexino

Authors :
L. Papp
M. Cribier
O. Smirnov
Fausto Ortica
Lino Miramonti
Alessandra Re
E. Litvinovich
G. Mention
V. Fischer
Gioacchino Ranucci
N. Rossi
S. Farinon
G. Bellini
R. Tartaglia
I. N. Machulin
Hui Wang
Marco Pallavicini
D. D'Angelo
F. von Feilitzsch
S. Schönert
R. B. Vogelaar
J. Winter
S. V. Sukhotin
M. Vivier
A. Caminata
N. Berton
Anton Empl
F. Gabriele
Y. Suvorov
Cristiano Galbiati
O. Zaimidoroga
Livia Ludhova
D. Franco
Matteo Agostini
A. M. Goretti
A. S. Chepurnov
C. Ghiano
V. N. Muratova
V. V. Kobychev
Caren Hagner
A. Pocar
G. Bonfini
L. Perasso
J. Maricic
Aldo Ianni
W. Maneschg
Kai Zuber
Aldo Romani
Denis Korablev
Frank Calaprice
S. Appel
Hardy Simgen
M. Obolensky
S. Davini
B. Neumair
P. Cavalcante
J. Gaffiot
B. Lehnert
L. Di Noto
Matthias Laubenstein
Michael Meyer
A.V. Etenko
K. Fomenko
M. Misiaszek
M. Göger-Neff
K. Altenmüller
Andrea Ianni
D. Bick
D. Bravo
D. Kryn
Jonathan M. Link
Sandra Zavatarelli
M. D. Skorokhvatov
G. Korga
Michael Wurm
Marcin Wójcik
B. Caccianiga
C. Veyssiere
L. Scola
Tobias Lachenmaier
E. Meroni
Marco Giammarchi
G. Testera
Paolo Lombardi
Michele Montuschi
A. V. Derbin
M. Durero
Lothar Oberauer
Thierry Lasserre
G. Zuzel
E. V. Hungerford
S. Marcocci
A. Sotnikov
Jay Burton Benziger
G. Lukyanchenko
M. Kaiser
F. Lombardi
A. Razeto
R. Musenich
N. Jonquères
M. Gromov
T. Houdy
Département de Physique Nucléaire (ex SPhN) (DPHN)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
AstroParticule et Cosmologie (APC (UMR_7164))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
EPJ Web Conf., 5th Roma International Conference on Astro-Particle physics, 5th Roma International Conference on Astro-Particle physics, Sep 2014, Noto, Italy. pp.01002, ⟨10.1051/epjconf/201612101002⟩, EPJ Web of Conferences, Vol 121, p 01002 (2016)
Publication Year :
2016
Publisher :
EDP Sciences, 2016.

Abstract

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy, sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection. These performances make it the ideal tool to accomplish a state-of-the-art experiment able to test unambiguously the long-standing issue of the existence of a sterile neutrino, as suggested by the several anomalous results accumulated over the past two decades, i.e. the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar neutrino experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on Chromium and Cerium, respectively, which deployed under the experiment, in a location foreseen on purpose at the time of the construction of the detector, will emit two intense beams of neutrinos (Cr) and anti-neutrinos (Ce). Interacting in the active volume of the liquid scintillator, each beam would create an unmistakable spatial wave pattern in case of oscillation of the nu_e (or nu̅_e) into the sterile state: such a pattern would be the smoking gun proving the existence of the new sterile member of the neutrino family. Otherwise, its absence will allow setting a very stringent limit on its existence.

Details

Language :
English
Database :
OpenAIRE
Journal :
EPJ Web Conf., 5th Roma International Conference on Astro-Particle physics, 5th Roma International Conference on Astro-Particle physics, Sep 2014, Noto, Italy. pp.01002, ⟨10.1051/epjconf/201612101002⟩, EPJ Web of Conferences, Vol 121, p 01002 (2016)
Accession number :
edsair.doi.dedup.....73652ca71ab8bc723a9e5f84ccc3d300