SimProp v2r3: Monte Carlo simulation code of UHECR propagation
Roberto Aloisio, Denise Boncioli, Armando di Matteo, Aurelio Grillo,, Sergio Petrera, Francesco Salamida
TL;DR
SimProp v2r3 is an advanced Monte Carlo simulation tool for modeling ultra-high energy cosmic ray propagation, offering enhanced flexibility with multiple models for background light, evolution, and interaction cross sections.
Contribution
It introduces a new version of SimProp with expanded model options for background light, evolution, and photodisintegration processes.
Findings
Enhanced modeling capabilities for cosmic ray propagation.
More accurate simulations due to diverse model options.
Improved understanding of UHECR interactions.
Abstract
We introduce the new version of SimProp, a Monte Carlo code for simulating the propagation of ultra-high energy cosmic rays in intergalactic space. This version, SimProp v2r3, allows the choice of many more models for the extragalactic background light spectrum and evolution and photodisintegration cross sections and branching ratios than previous versions of SimProp.
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