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Classification of electron and muon neutrino events for the ESSνSB near water Cherenkov detector using Graph Neural Networks
Consorcio ESS-bilbao, Parque Científico y Tecnológico de Bizkaia, Laida Bidea, Edificio 207-B, 48160 Derio, Bizkaia, Spain.
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging. The Oskar Klein Centre, AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm, Sweden.ORCID iD: 0000-0001-5948-9152
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging. The Oskar Klein Centre, AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm, Sweden.ORCID iD: 0000-0002-6071-8546
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging. The Oskar Klein Centre, AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm, Sweden.ORCID iD: 0000-0002-3525-8349
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Number of Authors: 972025 (English)In: Journal of Instrumentation, E-ISSN 1748-0221, Vol. 20, no 08, article id P08030Article in journal (Refereed) Published
Abstract [en]

In the effort to obtain a precise measurement of leptonic CP-violation with the ESSνSB experiment, accurate and fast reconstruction of detector events plays a pivotal role. In this work, we examine the possibility of replacing the currently proposed likelihood-based reconstruction method with an approach based on Graph Neural Networks (GNNs). As the likelihood-based reconstruction method is reasonably accurate but computationally expensive, one of the benefits of a Machine Learning (ML) based method is enabling fast event reconstruction in the detector development phase, allowing for easier investigation of the effects of changes to the detector design. Focusing on classification of flavour and interaction type in muon and electron events and muon- and electron neutrino interaction events, we demonstrate that the GNN reconstructs events with greater accuracy than the likelihood method for events with greater complexity, and with increased speed for all types of events. The GNN flavour classification of neutrino interaction events results in a true positive rate of 85.87 % (57.90 %) for muon (electron) neutrinos, compared to 35.55 % (0.21 %) for the likelihood-based method with identical constraints on the false positive rate, while the reconstruction speed is increased by a factor of 10<sup>4</sup>. Additionally, we investigate the key factors impacting reconstruction performance, and demonstrate how separation of events by pion production using another GNN classifier can benefit flavour classification.

Place, publisher, year, edition, pages
IOP Publishing , 2025. Vol. 20, no 08, article id P08030
Keywords [en]
Analysis and statistical methods, Cherenkov detectors, Neutrino detectors, Performance of High Energy Physics Detectors
National Category
Subatomic Physics Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-369733DOI: 10.1088/1748-0221/20/08/P08030ISI: 001572734900001Scopus ID: 2-s2.0-105014315317OAI: oai:DiVA.org:kth-369733DiVA, id: diva2:1997808
Note

QC 20250915

Available from: 2025-09-15 Created: 2025-09-15 Last updated: 2025-12-05Bibliographically approved

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Blennow, MattiasChoubey, SandhyaOhlsson, TommyVihonen, Sampsa

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