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dc.contributor.authorReininghaus, Maximilian
dc.contributor.authorSjöstrand, Torbjörn
dc.contributor.authorUtheim, Marius
dc.contributor.editorDe Mitri, I.
dc.contributor.editorBarbato, F. C. T.
dc.contributor.editorBoncioli, D.
dc.contributor.editorEvoli, C.
dc.contributor.editorPagliaroli, G.
dc.contributor.editorSalamida, F.
dc.date.accessioned2023-05-16T06:00:00Z
dc.date.available2023-05-16T06:00:00Z
dc.date.issued2023
dc.identifier.citationReininghaus, M., Sjöstrand, T., & Utheim, M. (2023). Pythia 8 as hadronic interaction model in air shower simulations. In I. De Mitri, F. C. T. Barbato, D. Boncioli, C. Evoli, G. Pagliaroli, & F. Salamida (Eds.), <i>Ultra High Energy Cosmic Rays (UHECR 2022)</i> (283, Article 05010). EDP Sciences. EPJ Web of Conferences. <a href="https://doi.org/10.1051/epjconf/202328305010" target="_blank">https://doi.org/10.1051/epjconf/202328305010</a>
dc.identifier.otherCONVID_183111912
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/86976
dc.description.abstractHadronic interaction models are a core ingredient of simulations of extensive air showers and pose the major source of uncertainties of predictions of air shower observables. Recently, Pythia 8, a hadronic interaction model popular in accelerator-based high-energy physics, became usable in air shower simulations as well. We have integrated Pythia 8 with its new capabilities into the air shower simulation framework CORSIKA 8. First results show significantly shallower shower development, which we attribute to higher cross-section predictions by the new simplified nuclear model of Pythia.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.ispartofUltra High Energy Cosmic Rays (UHECR 2022)
dc.relation.ispartofseriesEPJ Web of Conferences
dc.rightsCC BY 4.0
dc.titlePythia 8 as hadronic interaction model in air shower simulations
dc.typeconference paper
dc.identifier.urnURN:NBN:fi:jyu-202305163044
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.type.coarhttp://purl.org/coar/resource_type/c_5794
dc.description.reviewstatuspeerReviewed
dc.relation.issn2101-6275
dc.relation.volume283
dc.type.versionpublishedVersion
dc.rights.copyright© The Authors, published by EDP Sciences, 2023
dc.rights.accesslevelopenAccessfi
dc.type.publicationconferenceObject
dc.relation.conferenceInternational Symposium on Ultra High Energy Cosmic Rays
dc.subject.ysohiukkasfysiikka
dc.subject.ysosimulointi
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p4787
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1051/epjconf/202328305010
jyx.fundinginformationThe authors acknowledge support by the High Performance and Cloud Computing Group at the Zentrum für Datenverarbeitung of the University of Tübingen, the state of Baden-Württemberg through bwHPC and the German Research Foundation (DFG) through grant no. INST 37/935-1 FUGG.
dc.type.okmA4


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