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Marek P. Kowalski, Markus Ackermann, Jenni Adams, Sanjib Kumar Agarwalla et autres
Since its completion in 2011, the IceCube Neutrino Observatory has opened a new window on the extreme Universe. Building on its success in multi-messenger astronomy and particle physics, the collaboration is now pursuing a major extension: the IceCube-Gen2 facility. IceCube-Gen2 will be …
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Felix Riehn, Jean-Marco Alameddine, J. Albrecht, Antonio Augusto Alves Junior et autres
The simulation of particle cascades is an essential foundation for the analysis chains of many astroparticle physics experiments, irrespective of whether they investigate primarily charged cosmic rays, very high-energy photons or neutrinos, or even dark matter. The most widely used software for …
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Alfredo Ferrari, Ralph Engel, Anatoli Fedynitch, Mario Nicola Mazziotta et autres
Electromagnetic dissociation (EMD) is a well-known process that has been extensively studied using accelerator beams. However, the influence of EMD on cosmic-ray propagation in the atmosphere and galaxy remains unclear. For instance, understanding the origin of ultra-high energy cosmic rays requires knowledge …
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Chloé Gaudu, Jean-Marco Alameddine, J. Albrecht, Antonio Augusto Alves Junior et autres
The simulation of extensive air showers is pivotal for advancing our understanding of high-energy cosmic ray interactions in Earth's atmosphere. The CORSIKA 8 framework is being developed as a modern, flexible, and efficient tool for simulating these interactions with a variety of …
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T. K. Gaisser, Ralph Engel, Elisa Resconi
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Eun-Joo Ahn, Ralph Engel, T. K. Gaisser, Paolo Lipari et autres
The cosmic ray interaction event generator Sibyll is widely used in extensive air shower simulations for cosmic ray and neutrino experiments. Charmed particle production has been added to the Monte Carlo with a phenomenological, non-perturbative model that properly accounts for charm production …
David díEnterria, Ralph Engel, Thomas P. McCauley, T. Pierog
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Eun-Joo Ahn, Ralph Engel, T. K. Gaisser, Paolo Lipari et autres
The cosmic ray interaction event generator Sibyll is widely used in extensive air shower simulations. We describe in detail the properties of Sibyll 2.1 and the differences with the original version 1.7. The major structural improvements are the possibility to have multiple …
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Understanding hadronic multiparticle production is important for deriving the composition and energy spectrum of primary cosmic rays from air shower measurements at high energy. In this article, predictions of hadronic interaction models are discussed, emphasizing uncertainties and constraints due to model assumptions …
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Todor Stanev, D. Seckel, Ralph Engel
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