Novel techniques for alpha/beta pulse shape discrimination in Borexino
Creators: name: Basilico, D.
name: Bellini, G.
name: Benziger, J.
name: Biondi, R.
name: Caccianiga, B.
name: Calaprice, F.
name: Caminata, A.
name: Chepurnov, A.
name: D'Angelo, D.
name: Derbin, A.
name: Di Giacintov, A.
name: Di Marcello, V.
name: Ding, X. F.
name: Di Ludovico, A.
name: Di Noto, L.
name: Drachnev, I.
name: Franco, D.
name: Galbiati, C.
name: Ghiano, C.
name: Giammarchi, M.
name: Goretti, A.
name: Gromov, M.
name: Guffanti, D.
name: Ianni, Aldo
name: Ianni, Andrea
name: Jany, A.
name: Kobychev, V.
name: Korga, G.
name: Kumaran, S.
name: Laubenstein, M.
name: Litvinovich, E.
name: Lombardi, P.
name: Lomskaya, I.
name: Ludhova, L.
name: Machulin, I.
name: Martyn, J.
name: Meroni, E.
name: Miramonti, L.
name: Misiaszek, M.
name: Muratova, V.
name: Nugmanov, R.
name: Oberauer, L.
name: Orekhov, V.
name: Ortica, F.
name: Pallavicini, M.
name: Pelicci, L.
name: Penek, O.
name: Pietrofaccia, L.
name: Pilipenko, N.
name: Pocar, A.
name: Raikov, G.
name: Ranalli, M. T.
name: Ranucci, G.
name: Razeto, A.
name: Re, A.
name: Rossi, N.
name: Schoenert, S.
name: Semenov, D.
name: Settanta, G.
name: Skorokhvatov, M.
name: Singhal, A.
name: Smirnov, O.
name: Sotnikov, A.
name: Tartaglia, R.
name: Testera, G.
name: Unzhakov, E.
name: Vishneva, A.
name: Vogelaar, R. B.
name: von Feilitzsch, F.
name: Wojcik, M.
name: Wurm, M.
name: Zavatarelli, S.
name: Zuber, K.
name: Zuzel, G.
Publisher: name: Forschungzentrum Jülich
Year: 2023
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: arXiv (2023). doi:10.48550/arXiv.2310.11826
description: Borexino could efficiently distinguish between alpha and beta radiation in its liquid scintillator by the characteristic time profile of their scintillation pulse. This alpha/beta discrimination, first demonstrated at the tonne scale in the Counting Test Facility prototype, was used throughout the lifetime of the experiment between 2007 and 2021. With this method, alpha events are identified and subtracted from the beta-like solar neutrino events. This is particularly important in liquid scintillator as alpha scintillation is quenched many-fold. In Borexino, the prominent Po-210 decay peak was a background in the energy range of electrons scattered from Be-7 solar neutrinos. Optimal alpha-beta discrimination was achieved with a 'multi-layer perceptron neural network', which its 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 characterising 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 the key milestones in alpha/beta discrimination in Borexino as a term of comparison for current and future large liquid scintillator detectors
description: Published by arXiv