Study of proton capture on carbon-13 isotope at LUNA

被引：1
|
作者：
Rapagnani, David [1 ,2 ]
Skowronski, Jakub [3 ,4 ]
Boeltzig, Axel [5 ]
机构：
[1] Univ Napoli Federico II, Complesso Univ Monte Sant Angelo Via Cinthia 21, I-80125 Naples, Italy
[2] INFN Sez Napoli, Complesso Univ Monte Sant Angelo Via Cinthia 21, I-80125 Naples, Italy
[3] Univ Padua, Via Francesco Marzolo 8, I-35131 Padua, Italy
[4] INFN Sez Padova, Via Francesco Marzolo 8, I-35131 Padua, Italy
[5] Helmholtz Zentrum Dresden Rossendorf, Bautzner Landstr 400, D-01328 Dresden, Germany
来源：
28TH INTERNATIONAL NUCLEAR PHYSICS CONFERENCE, INPC 2022 | 2023年 / 2586卷
基金：
欧洲研究理事会;
关键词：
D O I：
10.1088/1742-6596/2586/1/012103
中图分类号：
TL [原子能技术]; O571 [原子核物理学];
学科分类号：
0827 ; 082701 ;
摘要：
C-13(p, gamma)N-14 is a key reaction in different stellar environments for which both accurate and precise measurements of its cross section are required to constraint stellar models. This is currently ongoing at the Laboratory for Underground Nuclear Astrophysics where in addition to the low-background environment, the use of different detection systems (HPGe and BGO detectors) and analysis techniques (Peak Shape Analysis and Sum Peak Method) allowed to perform reaction cross section measurements at the lowest energy ever. Both the setup employed in the measurements and the analysis performed are presented in this paper.
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页数：5
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