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Simulating radio emissions from particle showers in complex media with CORSIKA 8

P. J. WindischhoferDepartment of Physics , Enrico Fermi Institute , Kavli Institute for Cosmological Physics ,Jean-Marco AlameddineLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyJ. AlbrechtLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyA. A. AlvesUniversity of Cincinnati , Cincinnati , OH , United StatesJuan Ammerman YebraIMAPP , Radboud University Nijmegen , Nijmegen , The NetherlandsLuisa ArrabitoLaboratoire Univers et Particules de MontpellierDominik BaackLamarr Institute for Machine Learning and Artificial Intelligence , Dortmund , GermanyRui CesistaLaboratoire Univers & Particules de Montpellier , CNRS & Université de Montpellier ( UMR- 5299) , 34095 Montpellier , FranceAlan 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 , GermanyR. 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 GläserTechnische Universität Dortmund ( TU) , Department of Physics , Dortmund , GermanyMarvin GottowikKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyDieter HeckKarlsruhe Institute of Technology (KIT) , Institute for Astroparticle Physics (IAP) , Karlsruhe , GermanyT. HuegeVrije Universiteit Brussel , Astrophysical Institute , Brussels , BelgiumKarl-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. RhodeTechnische Universität Dortmund ( TU) , Department of Physics , 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. UlrichUniversity of Chicago , Chicago , IL 60637 , USABin YueBergische Universität Wuppertal , Department of Physics , Wuppertal , Germany
2025en
ABI

Annotatsiya

CORSIKA 8 is a modern Monte-Carlo simulation framework for particle showers in air and dense media. The calculation of shower-induced radio-emissions is a key element of the code, relevant for experiments targeting radio detection of cosmic rays and neutrinos, among others. In this contribution, we report on the unique capabilities of CORSIKA 8 to simulate the radio emission from showers developing in inhomogeneous media and the propagation of this radiation through these complex environments that cannot be properly treated with other methods. Several radio emission and propagation algorithms are provided by the framework, including the Endpoint and ZHS formalisms, numerical raytracing, and a new Green's function-based approach for a full-electrodynamics signal calculation provided by the Eisvogel package. We briefly review these approaches and show simulation results relevant for radio neutrino experiments operating in the Arctic and Antarctic, including the modeling of in-ice particle cascades and the characterization of the physics background arising from cosmic-ray air shower cores impacting the ice sheet.

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