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A convolutional neural network based cascade reconstruction for the IceCube Neutrino Observatory

  • The IceCube Collaboration
  • Loyola University Chicago
  • German Electron Synchrotron
  • University of Canterbury
  • Université libre de Bruxelles
  • University of Copenhagen
  • Stockholm University
  • University of Geneva
  • Karlsruhe Institute of Technology
  • University of Delaware
  • Harvard University
  • Marquette University
  • Pennsylvania State University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Massachusetts Institute of Technology
  • South Dakota School of Mines & Technology
  • University of Wisconsin-Madison
  • University of California at Irvine
  • Johannes Gutenberg University Mainz
  • University of California at Berkeley
  • Ohio State University
  • University of Wuppertal
  • Ruhr University Bochum
  • Technical University of Munich
  • University of Rochester
  • University of Maryland, College Park
  • University of Padua
  • Moscow Engineering Physics Institute
  • University of Kansas
  • Lawrence Berkeley National Laboratory
  • Uppsala University
  • RWTH Aachen University
  • University of Münster
  • Drexel University

Research output: Contribution to journalArticlepeer-review

73 Scopus citations

Abstract

Continued improvements on existing reconstruction methods are vital to the success of high-energy physics experiments, such as the IceCube Neutrino Observatory. In IceCube, further challenges arise as the detector is situated at the geographic South Pole where computational resources are limited. However, to perform real-time analyses and to issue alerts to telescopes around the world, powerful and fast reconstruction methods are desired. Deep neural networks can be extremely powerful, and their usage is computationally inexpensive once the networks are trained. These characteristics make a deep learning-based approach an excellent candidate for the application in IceCube. A reconstruction method based on convolutional architectures and hexagonally shaped kernels is presented. The presented method is robust towards systematic uncertainties in the simulation and has been tested on experimental data. In comparison to standard reconstruction methods in IceCube, it can improve upon the reconstruction accuracy, while reducing the time necessary to run the reconstruction by two to three orders of magnitude.

Original languageEnglish
Article numberP07041
JournalJournal of Instrumentation
Volume16
Issue number7
DOIs
StatePublished - Jul 2021

Keywords

  • Calibration
  • Cluster finding
  • Data analysis
  • Fitting methods
  • Neutrino detectors
  • Pattern recognition

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