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Sequential networks for cosmic ray simulations

dc.contributor.authorSampathkumar,Pranav
dc.contributor.authorAlves Junior,Augusto Antonio
dc.contributor.authorPierog,Tanguy
dc.contributor.authorUlrich,Ralf
dc.contributor.editorDemmler, Daniel
dc.contributor.editorKrupka, Daniel
dc.contributor.editorFederrath, Hannes
dc.date.accessioned2022-09-28T17:10:29Z
dc.date.available2022-09-28T17:10:29Z
dc.date.issued2022
dc.description.abstractA hybrid model of generating cosmic ray showers based on neural networks is presented. We show that the neural network learns the solution to the governing cascade equation in one dimension. We then use the neural network to generate the energy spectra at every height slice. Pitfalls of training to generate a single height slice is discussed, and we present a sequential model which can generate the entire shower from an initial table. Errors associated with the model and the potential to generate the full three dimensional distribution of the shower is discussed.en
dc.identifier.doi10.18420/inf2022_41
dc.identifier.isbn978-3-88579-720-3
dc.identifier.pissn1617-5468
dc.identifier.urihttps://dl.gi.de/handle/20.500.12116/39541
dc.language.isoen
dc.publisherGesellschaft für Informatik, Bonn
dc.relation.ispartofINFORMATIK 2022
dc.relation.ispartofseriesLecture Notes in Informatics (LNI) - Proceedings, Volume P-326
dc.subjectSequential Neural Networks
dc.subjectAstroparticle Physics
dc.subjectMonte Carlo Simulations
dc.titleSequential networks for cosmic ray simulationsen
gi.citation.endPage506
gi.citation.startPage499
gi.conference.date26.-30. September 2022
gi.conference.locationHamburg
gi.conference.sessiontitleWorkshop on Machine Learning for Astroparticle Physics and Astronomy (ml.astro)

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