Spallation reactions. A successful interplay between modeling and applications
J.-C. David

TL;DR
This paper reviews the history, modeling, and applications of spallation reactions, highlighting advances in theoretical understanding, model validation, and their importance in space and particle physics applications.
Contribution
It provides a comprehensive overview of spallation reaction modeling, benchmarking efforts, and discusses future development directions, emphasizing the progress made since early experiments.
Findings
High-quality spallation models have been developed with significant improvements.
Benchmarking shows many models now reliably reproduce experimental data.
Spallation modeling is crucial for applications in space, nuclear physics, and particle transport.
Abstract
The spallation reactions are a type of nuclear reaction which occur in space by interaction of the cosmic rays with interstellar bodies. The first spallation reactions induced with an accelerator took place in 1947 at the Berkeley cyclotron (University of California) with 200 MeV deuterons and 400 MeV alpha beams. They highlighted the multiple emission of neutrons and charged particles and the production of a large number of residual nuclei far different from the target nuclei. The same year R. Serber describes the reaction in two steps: a first and fast one with high-energy particle emission leading to an excited remnant nucleus, and a second one, much slower, the de-excitation of the remnant. In 2010 IAEA organized a worskhop to present the results of the most widely used spallation codes within a benchmark of spallation models. If one of the goals was to understand the deficiencies,…
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