AMS-02 on the International Space Station has been releasing data of
unprecedented accuracy. This poses new challenges for their interpretation.
In this paper, we refine the methodology to get a statistically sound determination of the
cosmic-ray propagation parameters. For this purpose, we
inspect the impact of nuclear cross-section uncertainties and energy correlations
in data systematic errors.
Fitting B/C cosmic-ray data in the AMS-02 era
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Pre-published on:
July 22, 2019
Published on:
July 02, 2021
Abstract
DOI: https://doi.org/10.22323/1.358.0054
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.