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@ARTICLE{Bieger:910200,
author = {Bieger, Lukas and Birkenfeld, Thilo and Blum, David and
Depnering, Wilfried and Enqvist, Timo and Enzmann, Heike and
Gao, Feng and Genster, Christoph and Göttel, Alexandre and
Grewing, Christian and Gromov, Maxim and Hackspacher, Paul
and Hagner, Caren and Heinz, Tobias and Kampmann, Philipp
and Karagounis, Michael and Kruth, Andre and Kuusiniemi,
Pasi and Lachenmaier, Tobias and Liebau, Daniel and Liu,
Runxuan and Loo, Kai and Ludhova, Livia and Meyhöfer, David
and Müller, Axel and Muralidharan, Pavithra and Oberauer,
Lothar and Othegraven, Rainer and Parkalian, Nina and Pei,
Yatian and Pilarczyk, Oliver and Rebber, Henning and Robens,
Markus and Roth, Christian and Sawatzki, Julia and
Schweizer, Konstantin and Settanta, Giulio and Slupecki,
Maciej and Smirnov, Oleg and Stahl, Achim and Steiger, Hans
and Steinmann, Jochen and Sterr, Tobias and Stock, Matthias
Raphael and Tang, Jian and Theisen, Eric and Tietzsch,
Alexander and Trzaska, Wladyslaw and van den Boom, Johannes
and van Waasen, Stefan and Vollbrecht, Cornelius and
Wiebusch, Christopher and Wonsak, Bjoern and Wurm, Michael
and Wysotzki, Christian and Xu, Yu and Yegin, Ugur and
Zambanini, Andre and Züfle, Jan},
title = {{P}otential for a precision measurement of solar pp
neutrinos in the {S}erappis experiment},
journal = {The European physical journal / C},
volume = {82},
number = {9},
issn = {1434-6044},
address = {Heidelberg},
publisher = {Springer},
reportid = {FZJ-2022-03678},
pages = {779},
year = {2022},
abstract = {The Serappis (SEarch for RAre PP-neutrinos In Scintillator)
project aims at a precision measurement of the flux of solar
pp neutrinos on the few-percent level. Such a measurement
will be a relevant contribution to the study of solar
neutrino oscillation parameters and a sensitive test of the
equilibrium between solar energy output in neutrinos and
electromagnetic radiation (solar luminosity constraint). The
concept of Serappis relies on a small organic liquid
scintillator detector (∼20 m$^3$) with excellent energy
resolution (∼2.5\% at 1 MeV), low internal background and
sufficient shielding from surrounding radioactivity. This
can be achieved by a minor upgrade of the OSIRIS facility at
the site of the JUNO neutrino experiment in southern China.
To go substantially beyond current accuracy levels for the
pp flux, an organic scintillator with ultra-low $^{14}$C
levels (below 10$^{−18}$) is required. The existing OSIRIS
detector andJUNO infrastructure will be instrumental in
identifying suitable scintillator materials, offering a
unique chance for a low-budget high-precision measurement of
a fundamental property of our Sun that will be otherwise
hard to access.},
cin = {IKP-2 / ZEA-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104 / I:(DE-Juel1)ZEA-2-20090406},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000849219200004},
doi = {10.1140/epjc/s10052-022-10725-y},
url = {https://juser.fz-juelich.de/record/910200},
}