A convolutional neural network based cascade reconstruction for the IceCube Neutrino Observatory
Creators
- 1. Department of Physics, Loyola University Chicago, Chicago, IL 60660 (United States)
- 2. DESY, D-15738 Zeuthen (Germany)
- 3. Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch (New Zealand)
- 4. Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels (Belgium)
- 5. Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen (Denmark)
- 6. Oskar Klein Centre and Department of Physics, Stockholm University, SE-10691 Stockholm (Sweden)
- 7. Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève (Switzerland)
- 8. Karlsruhe Institute of Technology, Institute for Astroparticle Physics, D-76021 Karlsruhe (Germany)
- 9. Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE 19716 (United States)
- 10. Department of Physics and Laboratory for Particle Physics and Cosmology Harvard University, Cambridge, MA 02138 (United States)
- 11. Department of Physics, Marquette University, Milwaukee, WI, 53201 (United States)
- 12. Department of Physics, Pennsylvania State University, University Park, PA 16802 (United States)
- 13. Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen (Germany)
- 14. Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)
- 15. Physics Department, South Dakota School of Mines and Technology, Rapid City, SD 57701 (United States)
Description
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. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1748-0221/16/07/P07041Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Instrumentation
- Journal Volume
- 16
- Journal Issue
- 07
- Journal Page Range
- [38 p.]
- ISSN
- 1748-0221
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53081990
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- ACCURACY; COMPUTERIZED SIMULATION; HIGH ENERGY PHYSICS; ICECUBE NEUTRINO DETECTOR; MACHINE LEARNING; NEURAL NETWORKS; NEUTRINOS; TELESCOPES
- Descriptors DEC
- ALGORITHMS; ARTIFICIAL INTELLIGENCE; ELEMENTARY PARTICLES; FERMIONS; LEARNING; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL LOGIC; MEASURING INSTRUMENTS; NEUTRINO DETECTORS; PHYSICS; RADIATION DETECTORS; SIMULATION
Optional Information
- Collaborations
- IceCube Collaboration