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Graph Neural Networks for low-energy event classification & reconstruction in IceCube

40Citations signalées, ce qui n’est pas une note de qualité
60Institutions déclarées
15Pays d’affiliation déclarés

Rattachement africain : us, nz, ca, be, dk, se, de, it, au, kr, bd, tw, jp, ch, gb. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

Abstract IceCube, a cubic-kilometer array of optical sensors built to detect atmospheric and astrophysical neutrinos between 1 GeV and 1 PeV, is deployed 1.45 km to 2.45 km below the surface of the ice sheet at the South Pole. The classification and reconstruction of events from the in-ice detectors play a central role in the analysis of data from IceCube. Reconstructing and classifying events is a challenge due to the irregular detector geometry, inhomogeneous scattering and absorption of light in the ice and, below 100 GeV, the relatively low number of signal photons produced per event. To address this challenge, it is possible to represent IceCube events as point cloud graphs and use a Graph Neural Network (GNN) as the classification and reconstruction method. The GNN is capable of distinguishing neutrino events from cosmic-ray backgrounds, classifying different neutrino event types, and reconstructing the deposited energy, direction and interaction vertex. Based on simulation, we provide a comparison in the 1 GeV–100 GeV energy range to the current state-of-the-art maximum likelihood techniques used in current IceCube analyses, including the effects of known systematic uncertainties. For neutrino event classification, the GNN increases the signal efficiency by 18% at a fixed background rate, compared to current IceCube methods. Alternatively, the GNN offers a reduction of the background (i.e. false positive) rate by over a factor 8 (to below half a percent) at a fixed signal efficiency. For the reconstruction of energy, direction, and interaction vertex, the resolution improves by an average of 13%–20% compared to current maximum likelihood techniques in the energy range of 1 GeV–30 GeV. The GNN, when run on a GPU, is capable of processing IceCube events at a rate nearly double of the median IceCube trigger rate of 2.7 kHz, which opens the possibility of using low energy neutrinos in online searches for transient events.

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Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.

Titre Crossref
Graph Neural Networks for low-energy event classification & reconstruction in IceCube
Date Crossref
01/11/2022
Éditeur
IOP Publishing
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

Loyola University ChicagoUniversity of CanterburyUniversity of AlbertaUniversité Libre de BruxellesUniversity of CopenhagenStockholm UniversityTU Dortmund UniversityKarlsruhe Institute of TechnologyUniversity of DelawareMarquette UniversityPennsylvania State UniversityFriedrich-Alexander-Universität Erlangen-NürnbergInstitute of Particle PhysicsUniversity of Wisconsin–MadisonMassachusetts Institute of TechnologySouth Dakota School of Mines and TechnologyUniversity of California, IrvineUniversity of California, BerkeleyThe Ohio State UniversityUniversity of WuppertalRuhr University BochumUppsala UniversityTechnical University of MunichUniversity of RochesterUniversity of Maryland, College ParkUniversity of PaduaUniversity of KansasLawrence Berkeley National LaboratoryRWTH Aachen UniversityJohannes Gutenberg University MainzGeorgia Institute of TechnologyThe University of AdelaideUniversity of MünsterDrexel UniversityStony Brook UniversitySungkyunkwan UniversityMichigan State UniversityVrije Universiteit BrusselColumbia UniversityUniversity of AlabamaUCLouvainSouthern University and Agricultural and Mechanical CollegeSouthern UniversityInstitute of Physics, Academia SinicaHumboldt-Universität zu BerlinUniversity of Wisconsin SystemQueen's UniversityChiba UniversityClark Atlanta UniversityThe University of Texas at ArlingtonUniversity of GenevaUniversity of California, Los AngelesYale UniversityMercer UniversityGhent UniversityUniversity of Alaska AnchorageUniversity of UtahUniversity of OxfordScience OxfordUniversity of Wisconsin–River Falls

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Astrophysics and Cosmic PhenomenaEarthquake Detection and AnalysisNeutrino Physics Research

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