Year: 2025
Type: conference-paper
Abstract: We present CRPropa 3.3, the latest release of the publicly available Monte Carlo framework for simulating the propagation of high-energy particles in astrophysical environments. This version introduces significant extensions that enables multi-messenger studies across a broad energy range, from GeV to ZeV. New features include explicit time tracking, time-dependent advection fields, and support for position-dependent radiation backgrounds, for more realistic simulations of Galactic and extragalactic propagation. Nuclear cross sections have been updated and expanded up to lead (Z=82). We illustrate some of these new features, including acceleration at moving shocks and gamma-ray propagation in the interstellar radiation field. Together, these improvements establish CRPropa 3.3 as a comprehensive tool for modelling cosmic rays, gamma rays, and their secondaries in structured, time-dependent environments, setting the stage for next-generation multi-messenger astrophysics.
DOI: 10.22323/1.501.0964
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: G1892388310, G338497233, G432818845, MultiMessenger Ansatz zur Suche nach den Quellen der kosmischen Strahlung, Verbundprojekt 05A2023 - AUGER: Das Pierre-Auger-Projekt: Erdgebundene Messung der kosmischen Strahlung höchster Energien bis über 10^20 eV. Teilprojekt 2., G6141822678, G702601109, G7080048889, EXC 2121: Quantum Universe, Verbundprojekt 05A2020 - AUGER: Das Pierre-Auger-Projekt:Messungen der kosmischen Energien von über 10^(20) eV. Teilprojekt 4, Verbundprojekt 05A2020 - AUGER: Das Pierre-Auger-Projekt: Messungen der kosmischen Energien von über 10^(20) eV. Teilprojekt 1
OpenAlex ID: W4414438222
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