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CORSIKA 8 -- the next-generation air shower simulation framework

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arxiv 2208.14240 v2 pith:2YKZIUNQ submitted 2022-08-30 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords corsikasimulationexampleframeworkshowersadaptationapplicationscherenkov
verification ladder T0 review T1 audit T2 compute T3 formal
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For more than 20 years, the community has heavily relied on CORSIKA for the simulation of extensive air showers, their Cherenkov light emission and their radio signals. While tremendously successful, the Fortran-based monolithic design of CORSIKA up to version 7 limits adaptation to new experimental needs, for example, in complex scenarios where showers transition from air into dense media, and to new computing paradigms such as the use of multi-core and GPU parallelization. With CORSIKA 8, we have reimplemented the core functionality of CORSIKA in a modern, modular, C++-based simulation framework, and successfully validated it against CORSIKA 7. Here, we discuss the philosophy of CORSIKA 8, showcase some example applications, and present the current state of implementation as well as the plans for the future.

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Cited by 1 Pith paper

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  1. Probing the Cosmic Ray Background of Gamma-Ray Astronomy with Hadron Colliders

    astro-ph.HE 2025-09 conditional novelty 5.0 of 10

    Only forward neutral pions carrying a large fraction of the cosmic-ray energy mimic gamma-ray showers, and LHCf/RHICf cover the exact pseudorapidity range needed to test the models.

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