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A large scientific community depends on the precise modelling of complexprocesses in particle cascades in various types of matter. These models areused most prevalently in cosmic-ray physics, astrophysical-neutrino physics,and gamma-ray astronomy. In this white paper, we summarize the necessary stepsto ensure the evolution and future availability of optimal simulation tools.The purpose of this document is not to act as a strict blueprint fornext-generation software, but to provide guidance for the vital aspects of itsdesign. The topics considered here are driven by physics and scientificapplications. Furthermore, the main consequences of implementation decisions onperformance are outlined. We highlight the computational performance as animportant aspect guiding the design since future scientific applications willheavily depend on an efficient use of computational resources.

Towards a Next Generation of CORSIKA: A Framework for the Simulation of Particle Cascades in Astroparticle Physics