Novel thick-target inverse kinematics method for the astrophysical C+C fusion reaction
Nuclear Science and Techniques, ISSN: 2210-3147, Vol: 35, Issue: 11
2024
- 2Citations
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Citations2
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Article Description
The 12C+12C fusion is one of the most important reactions in modern nuclear astrophysics. The trend and magnitude of the reaction rate within the Gamow window strongly influence various astrophysical processes. However, direct measurement of this reaction is extremely difficult, which makes it necessary to develop indirect methods. In this study, the 23Na+p reaction system was used to study the compound nucleus 24Mg. We employed a thick-target inverse kinematics method combined with the γ-charged-particle coincidence technique to measure the proton and α exit channels of 24Mg. Technical details of the 23Na+p thick-target inverse kinematics experiment and analysis are presented herein.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85207694988&origin=inward; http://dx.doi.org/10.1007/s41365-024-01573-4; https://link.springer.com/10.1007/s41365-024-01573-4; https://dx.doi.org/10.1007/s41365-024-01573-4; https://link.springer.com/article/10.1007/s41365-024-01573-4; http://sciencechina.cn/gw.jsp?action=cited_outline.jsp&type=1&id=7859457&internal_id=7859457&from=elsevier
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