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This content will become publicly available on November 25, 2022

Title: The status and future of direct nuclear reaction measurements for stellar burning
Abstract The study of stellar burning began just over 100 years ago. Nonetheless, we do not yet have a detailed picture of the nucleosynthesis within stars and how nucleosynthesis impacts stellar structure and the remnants of stellar evolution. Achieving this understanding will require precise direct measurements of the nuclear reactions involved. This report summarizes the status of direct measurements for stellar burning, focusing on developments of the last couple of decades, and offering a prospectus of near-future developments.
Authors:
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Award ID(s):
2011890 1913746
Publication Date:
NSF-PAR ID:
10309720
Journal Name:
Journal of Physics G: Nuclear and Particle Physics
Volume:
49
Issue:
1
ISSN:
0954-3899
Sponsoring Org:
National Science Foundation
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