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@ARTICLE{Basilico:1038442,
author = {Basilico, D. and Bellini, G. and Benziger, J. and Biondi,
R. and Caccianiga, B. and Calaprice, F. and Caminata, A. and
Chepurnov, A. and D’Angelo, D. and Derbin, A. and Di
Giacinto, A. and Di Marcello, V. and Ding, X. F. and Di
Ludovico, A. and Di Noto, L. and Drachnev, I. and Franco, D.
and Galbiati, C. and Ghiano, C. and Giammarchi, M. and
Goretti, A. and Gromov, M. and Guffanti, D. and Ianni, Aldo
and Ianni, Andrea and Jany, A. and Kobychev, V. and Korga,
G. and Kumaran, S. and Laubenstein, M. and Litvinovich, E.
and Lombardi, P. and Lomskaya, I. and Ludhova, L. and
Machulin, I. and Martyn, J. and Meroni, E. and Miramonti, L.
and Misiaszek, M. and Muratova, V. and Nugmanov, R. and
Oberauer, L. and Orekhov, V. and Ortica, F. and Pallavicini,
M. and Pelicci, L. and Penek, Ö. and Pietrofaccia, L. and
Pilipenko, N. and Pocar, A. and Raikov, G. and Ranalli, M.
T. and Ranucci, G. and Razeto, A. and Re, A. and Rossi, N.
and Schönert, S. and Semenov, D. and Settanta, G. and
Skorokhvatov, M. and Singhal, A. and Smirnov, O. and
Sotnikov, A. and Tartaglia, R. and Testera, G. and Unzhakov,
E. and Vishneva, A. and Vogelaar, R. B. and von Feilitzsch,
F. and Wojcik, M. and Wurm, M. and Zavatarelli, S. and
Zuber, K. and Zuzel, G.},
title = {{O}ptimized α / β pulse shape discrimination in
{B}orexino},
journal = {Physical review / D},
volume = {109},
number = {11},
issn = {2470-0010},
address = {Ridge, NY},
publisher = {American Physical Society},
reportid = {FZJ-2025-01438},
pages = {112014},
year = {2024},
abstract = {Borexino could efficiently distinguish between 𝛼 and
𝛽 radiation in its liquid scintillator by the
characteristic time profile of its scintillation pulse. This
𝛼/𝛽 discrimination, first demonstrated on the ton
scale in the counting test facility prototype, was used
throughout the lifetime of the experiment between 2007 and
2021. With this method, the 𝛼 events are identified and
subtracted from the solar neutrino events similar to 𝛽.
This is particularly important in liquid scintillators, as
the 𝛼 scintillation is strongly quenched. In Borexino,
the prominent 210 Po decay peak was a background in the
energy range of electrons scattered from 7 Be solar
neutrinos. Optimal 𝛼/𝛽 discrimination was achieved
with a multilayer perceptron neural network, with a higher
ability to leverage the timing information of the
scintillation photons detected by the photomultiplier tubes.
An event-by-event, high efficiency, stable, and uniform
pulse shape discrimination was essential in characterizing
the spatial distribution of background in the detector. This
benefited most Borexino measurements, including solar
neutrinos in the 𝑝𝑝 chain and the first direct
observation of the CNO cycle in the Sun. This paper presents
key milestones in 𝛼/𝛽 discrimination in Borexino as a
term of comparison for current and future large liquid
scintillator detectors.},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16},
UT = {WOS:001252569300001},
doi = {10.1103/PhysRevD.109.112014},
url = {https://juser.fz-juelich.de/record/1038442},
}