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The $^{144}$Ce source for SOX

Authors :
A. Pocar
O. Smirnov
Marcin Wójcik
A. Caminata
Matthias Laubenstein
E. V. Unzhakov
D. Kryn
Aldo Ianni
T. Lasserre
S. Appel
L. Papp
M. D. Skorokhvatov
Michael Wurm
M. Vivier
E. Meroni
K. Jedrzejczak
Fausto Ortica
Z. Yokley
A. V. Derbin
J. Thurn
B. Caccianiga
D. A. Semenov
S. Farinon
M. Obolensky
B. Lehnert
L. Scola
C. Veyssiere
Kai Zuber
K. Choi
N. Jonqueres
M. Gromov
Lothar Oberauer
S. Weinz
Tobias Lachenmaier
Marco Giammarchi
Alessandra Re
T. Houdy
S. Manecki
G. Testera
Cristiano Galbiati
J. Maricic
E. Litvinovich
G. Mention
N. Rossi
Jay Burton Benziger
I. N. Machulin
L. Perasso
N. Berton
Marco Pallavicini
D. D'Angelo
V. Fischer
G. Bonfini
Denis Korablev
C. Ghiano
Matteo Agostini
F. Lombardi
A. Razeto
Frank Calaprice
Suvorov
M. Cribier
Hardy Simgen
M. Kaiser
M. Goeger-Neff
R. B. Vogelaar
S. Davini
I. S. Drachnev
J. Winter
B. Neumair
Livia Ludhova
G. Korga
D. Franco
A. M. Goretti
A. S. Chepurnov
M. S. Meyer
K. Fomenko
G. Lukyanchenko
M. Durero
J. M. Link
R. Tartaglia
Paolo Lombardi
S. V. Sukhotin
F. von Feilitzsch
Lino Miramonti
O. Zaimidoroga
H. Wang
Aldo Romani
L. Di Noto
W. Maneschg
V. V. Kobychev
Michele Montuschi
G. Bellini
Caren Hagner
R. Roncin
P. Cavalcante
M. Misiaszek
Kornoukhov
S. Schönert
A.V. Etenko
D. Bravo
Andrea Ianni
D. Bick
Sandra Zavatarelli
Gioacchino Ranucci
J. Gaffiot
E. V. Hungerford
A. Sotnikov
F. Gabriele
V. N. Muratova
R. Musenich
G. Zuzel
S. Marcocci
M. Toropova
K. Altenmüller
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))
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)
Borexino
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)
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)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
J.Phys.Conf.Ser., 1st International Conference on Particle Physics and Astrophysics, 1st International Conference on Particle Physics and Astrophysics, Oct 2015, Moscow, Russia. pp.012032, ⟨10.1088/1742-6596/675/1/012032⟩, Journal of physics / Conference Series 675(1), 012032-(2016). doi:10.1088/1742-6596/675/1/012032, The International Conference on Particle Physics and Astrophysics Moscow, ICPPA-2015, Moscow, Russia, 2015-10-05-2015-10-10
Publication Year :
2015
Publisher :
HAL CCSD, 2015.

Abstract

International audience; The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the (144)Ce-(144)Pr pair at secular equilibrium. It will be produced at FSUE “Mayak” PA using spent nuclear fuel. It will then be shielded and packed according to international regulation and shipped to LNGS across Europe. Knowledge of the Cerium antineutrino generator (CeANG) parameters is crucial for SOX as it can strongly impact the experiment sensitivity. Several apparatuses are being used or designed to characterize CeANG activity, radioactive emission and content. An overview of the measurements performed so far is presented here.

Details

Language :
English
Database :
OpenAIRE
Journal :
J.Phys.Conf.Ser., 1st International Conference on Particle Physics and Astrophysics, 1st International Conference on Particle Physics and Astrophysics, Oct 2015, Moscow, Russia. pp.012032, ⟨10.1088/1742-6596/675/1/012032⟩, Journal of physics / Conference Series 675(1), 012032-(2016). doi:10.1088/1742-6596/675/1/012032, The International Conference on Particle Physics and Astrophysics Moscow, ICPPA-2015, Moscow, Russia, 2015-10-05-2015-10-10
Accession number :
edsair.doi.dedup.....d34e81b7a4d79cfd0c490c2a853bfa7f