Conditional normalizing flows for IceCube event reconstruction ...

The IceCube Neutrino Observatory is a cubic-kilometer high-energy neutrino detector deployed in the Antarctic ice. Two major event classes are charged-current electron and muon neutrino interactions. In this contribution, we discuss the inference of direction and energy for these classes using condi...

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Main Author: Glüsenkamp, Thorsten
Format: Article in Journal/Newspaper
Language:unknown
Published: arXiv 2023
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.2309.16380
https://arxiv.org/abs/2309.16380
id ftdatacite:10.48550/arxiv.2309.16380
record_format openpolar
spelling ftdatacite:10.48550/arxiv.2309.16380 2023-11-05T03:36:58+01:00 Conditional normalizing flows for IceCube event reconstruction ... Glüsenkamp, Thorsten 2023 https://dx.doi.org/10.48550/arxiv.2309.16380 https://arxiv.org/abs/2309.16380 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM Artificial Intelligence cs.AI High Energy Physics - Experiment hep-ex FOS Physical sciences FOS Computer and information sciences Article article CreativeWork Preprint 2023 ftdatacite https://doi.org/10.48550/arxiv.2309.16380 2023-10-09T11:10:04Z The IceCube Neutrino Observatory is a cubic-kilometer high-energy neutrino detector deployed in the Antarctic ice. Two major event classes are charged-current electron and muon neutrino interactions. In this contribution, we discuss the inference of direction and energy for these classes using conditional normalizing flows. They allow to derive a posterior distribution for each individual event based on the raw data that can include systematic uncertainties, which makes them very promising for next-generation reconstructions. For each normalizing flow we use the differential entropy and the KL-divergence to its maximum entropy approximation to interpret the results. The normalizing flows correctly incorporate complex optical properties of the Antarctic ice and their relation to the embedded detector. For showers, the differential entropy increases in regions of high photon absorption and decreases in clear ice. For muons, the differential entropy strongly correlates with the contained track length. Coverage ... : Presented at the 38th International Cosmic Ray Conference (ICRC2023). See arXiv:2307.13047 for all IceCube contributions ... Article in Journal/Newspaper Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic High Energy Astrophysical Phenomena astro-ph.HE
Instrumentation and Methods for Astrophysics astro-ph.IM
Artificial Intelligence cs.AI
High Energy Physics - Experiment hep-ex
FOS Physical sciences
FOS Computer and information sciences
spellingShingle High Energy Astrophysical Phenomena astro-ph.HE
Instrumentation and Methods for Astrophysics astro-ph.IM
Artificial Intelligence cs.AI
High Energy Physics - Experiment hep-ex
FOS Physical sciences
FOS Computer and information sciences
Glüsenkamp, Thorsten
Conditional normalizing flows for IceCube event reconstruction ...
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
Instrumentation and Methods for Astrophysics astro-ph.IM
Artificial Intelligence cs.AI
High Energy Physics - Experiment hep-ex
FOS Physical sciences
FOS Computer and information sciences
description The IceCube Neutrino Observatory is a cubic-kilometer high-energy neutrino detector deployed in the Antarctic ice. Two major event classes are charged-current electron and muon neutrino interactions. In this contribution, we discuss the inference of direction and energy for these classes using conditional normalizing flows. They allow to derive a posterior distribution for each individual event based on the raw data that can include systematic uncertainties, which makes them very promising for next-generation reconstructions. For each normalizing flow we use the differential entropy and the KL-divergence to its maximum entropy approximation to interpret the results. The normalizing flows correctly incorporate complex optical properties of the Antarctic ice and their relation to the embedded detector. For showers, the differential entropy increases in regions of high photon absorption and decreases in clear ice. For muons, the differential entropy strongly correlates with the contained track length. Coverage ... : Presented at the 38th International Cosmic Ray Conference (ICRC2023). See arXiv:2307.13047 for all IceCube contributions ...
format Article in Journal/Newspaper
author Glüsenkamp, Thorsten
author_facet Glüsenkamp, Thorsten
author_sort Glüsenkamp, Thorsten
title Conditional normalizing flows for IceCube event reconstruction ...
title_short Conditional normalizing flows for IceCube event reconstruction ...
title_full Conditional normalizing flows for IceCube event reconstruction ...
title_fullStr Conditional normalizing flows for IceCube event reconstruction ...
title_full_unstemmed Conditional normalizing flows for IceCube event reconstruction ...
title_sort conditional normalizing flows for icecube event reconstruction ...
publisher arXiv
publishDate 2023
url https://dx.doi.org/10.48550/arxiv.2309.16380
https://arxiv.org/abs/2309.16380
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.2309.16380
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