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Simulating radio emission from extensive air showers with CORSIKA 8

Marvin GottowikKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyJean-Marco AlameddineTechnische Universität Dortmund ( TU) , Department of Physics , Dortmund , GermanyJ. AlbrechtLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyA. A. AlvesKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyJuan Ammerman YebraIMAPP , Radboud University Nijmegen , Nijmegen , The NetherlandsLuisa ArrabitoLaboratoire Univers et Particules de MontpellierDominik BaackTechnische Universität Dortmund ( TU) , Department of Physics , Dortmund , GermanyRui CesistaLaboratoire Univers et Particules de MontpellierAlan ColemanUppsala University , Department of Physics and Astronomy , Uppsala , SwedenCosmin DeaconuDepartment of Physics , Enrico Fermi Institute , Kavli Institute for Cosmological Physics ,Hans DembinskiLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyDominik ElsässerLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyRalph EngelKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyAlice FaureLaboratoire Univers & Particules de Montpellier , CNRS & Université de Montpellier ( UMR- 5299) , 34095 Montpellier , FranceAlfredo FerrariKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyChloé GauduBergische Universität Wuppertal , Department of Physics , Wuppertal , GermanyChristian GläserUppsala University , Department of Physics and Astronomy , Uppsala , SwedenDieter HeckKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyT. HuegeKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyKarl-Heinz KampertBergische Universität Wuppertal , Department of Physics , Wuppertal , GermanyN. KarastathisKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyL. NellenUniversidad Nacional Autónoma de México (UNAM) , Instituto de Ciencias Nucleares , Méx- ico , MéxicoDavid ParelloUniversité de MontpellierTanguy PierogKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyRemy PrecheltUniversity of Hawai'i at Manoa , Department of Physics and Astronomy , Honolulu , USAMaximilian ReininghausW. RhodeLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyFelix RiehnTechnische Universität Dortmund ( TU) , Department of Physics , Dortmund , GermanyMaximilian SackelTechnische Universität Dortmund ( TU) , Department of Physics , Dortmund , GermanyPranav SampathkumarKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyAlexander SandrockBergische Universität Wuppertal , Department of Physics , Wuppertal , GermanyJan SoedingreksoLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyR. UlrichKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyP. J. WindischhoferUniversity of Chicago , Chicago , IL 60637 , USABin YueBergische Universität Wuppertal , Department of Physics , Wuppertal , Germany
2025en
ABI

Аннотация

CORSIKA 8 is a modern, flexible framework for simulating particle cascades in air and dense media, allowing for fully customizable shower simulations. The radio module autonomously handles electric field calculations and propagation to observer locations. It supports simultaneous simulations with both the "Endpoint formalism" as implemented in CoREAS and the "ZHS" algorithm from ZHAireS. In this contribution, we validate the radio module by comparing air-shower simulations in CORSIKA 8, CORSIKA 7, and ZHAireS. We investigate the impact of simulation parameters, such as the step size of particle tracks, on the resulting radio signals and perform a detailed comparison of the "Endpoints" and "ZHS" formalisms. For the same underlying showers simulated with CORSIKA 8 with optimized step sizes, both formalisms converge to the same radiation energy within 2%. For CORSIKA 8 and CORSIKA 7, agreement on the radiation energy is better than 10% in the 30–80 MHz band and improves to better than 2% for 50–350 MHz. This consistency provides further confirmation of the accuracy of microscopic air-shower radio emission simulations which is crucial for precise energy scale estimations using radio detection.

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