Pythia 8 as hadronic interaction model in air shower simulations
dc.contributor.author | Reininghaus, Maximilian | |
dc.contributor.author | Sjöstrand, Torbjörn | |
dc.contributor.author | Utheim, Marius | |
dc.contributor.editor | De Mitri, I. | |
dc.contributor.editor | Barbato, F. C. T. | |
dc.contributor.editor | Boncioli, D. | |
dc.contributor.editor | Evoli, C. | |
dc.contributor.editor | Pagliaroli, G. | |
dc.contributor.editor | Salamida, F. | |
dc.date.accessioned | 2023-05-16T06:00:00Z | |
dc.date.available | 2023-05-16T06:00:00Z | |
dc.date.issued | 2023 | |
dc.identifier.citation | Reininghaus, 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.other | CONVID_183111912 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/86976 | |
dc.description.abstract | Hadronic 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.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | EDP Sciences | |
dc.relation.ispartof | Ultra High Energy Cosmic Rays (UHECR 2022) | |
dc.relation.ispartofseries | EPJ Web of Conferences | |
dc.rights | CC BY 4.0 | |
dc.title | Pythia 8 as hadronic interaction model in air shower simulations | |
dc.type | conference paper | |
dc.identifier.urn | URN:NBN:fi:jyu-202305163044 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/ConferencePaper | |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2101-6275 | |
dc.relation.volume | 283 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © The Authors, published by EDP Sciences, 2023 | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | conferenceObject | |
dc.relation.conference | International Symposium on Ultra High Energy Cosmic Rays | |
dc.subject.yso | hiukkasfysiikka | |
dc.subject.yso | simulointi | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4787 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1051/epjconf/202328305010 | |
jyx.fundinginformation | The 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.okm | A4 |