Measurement of the mass-changing, charge-changing and production cross sections of 11C, 11B and 10B nuclei in 12C+p interactions at 13.5 GeV/c per nucleon
Abstract
We report results from a 2018 pilot run to study the feasibility of nuclear fragmentation measurements with the NA61/SHINE experiment at the CERN SPS. These results are important for the interpretation of the production of light secondary cosmic-ray nuclei (Li, Be, and B) in the Galaxy. The specific focus here is on cross sections important for the production of boron in the Galaxy from the interactions of 12C nuclei with hydrogen in the interstellar medium, including the contribution from the decay of the short-lived 11C fragments. The data were taken with the secondary 12C beam at beam momentum of 13.5 GeV/c per nucleon and two fixed targets, polyethylene (CH2) and graphite (C), from which we derive the cross sections of carbon on hydrogen. We present the measurement of the fragmentation cross sections of 11C, 11B, and 10B as well as the mass- and charge-changing cross sections.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.