Issue |
EPJ Web Conf.
Volume 279, 2023
Nuclear Physics in Astrophysics – X (NPA-X 2022)
|
|
---|---|---|
Article Number | 03002 | |
Number of page(s) | 5 | |
Section | Quiescent Phases of Stellar Evolution | |
DOI | https://doi.org/10.1051/epjconf/202327903002 | |
Published online | 22 March 2023 |
https://doi.org/10.1051/epjconf/202327903002
Low-energy Cross Section Measurements of 12C(p, γ) Deep Underground at LUNA
1 Università degli Studi di Padova and INFN, Sezione di Padova, Via Francesco Marzolo 8, 35131 Padova, Italy
2 Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstraße 400, 01328 Dresden, Germany
* e-mail: a.boeltzig@hzdr.de
Published online: 22 March 2023
The 12C(p, γ)13N reaction cross section is currently under investigation in the low-background environment of the Laboratory for Underground Nuclear Astrophysics (LUNA). It is being studied using different types of solid targets, and employing two complementary detection techniques: HPGe spectroscopy and activation counting. To reduce systematic uncertainties, targets have been accurately characterized and their degradation under the intense beam of the LUNA-400 accelerator monitored. We present the experimental techniques and the corresponding analyses used to extract the reaction cross section.
© The Authors, published by EDP Sciences, 2023
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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