| Issue |
EPJ Web Conf.
Volume 165, 2017
Nuclear Physics in Astrophysics VIII (NPA8 2017)
|
|
|---|---|---|
| Article Number | 01006 | |
| Number of page(s) | 4 | |
| DOI | https://doi.org/10.1051/epjconf/201716501006 | |
| Published online | 30 December 2017 | |
https://doi.org/10.1051/epjconf/201716501006
23Na(p,γ)24Mg Cross Section Measurements
1 University of Notre Dame, Notre Dame, USA and Joint Institute for Nuclear Astrophysics (JINA)
2 Gran Sasso Science Institute (GSSI), L’Aquila, Italy
3 Università degli Studi di Napoli “Federico II” and INFN Sezione di Napoli, Naples, Italy
4 INFN Laboratori Nazionali del Gran Sasso, Assergi, Italy
* e-mail: axel.boeltzig@nd.edu
Published online: 30 December 2017
As a link between the NeNa and MgAl cycles in stellar burning, the reaction 23Na(p,γ)24Mg is of interest for various astrophysical scenarios, such as AGB stars. A combined effort at the Laboratory for Underground Nuclear Astrophysics (LUNA) and the Nuclear Science Laboratory (NSL) at the University of Notre Dame aims at a cross section determination for the this reaction, to constrain the astrophysical reaction rate by improving the knowledge of the resonance strengths and the non-resonant component. Experiments at LUNA benefit from the underground location at the Gran Sasso National Laboratory which allows for the measurement of resonances at low energies with high sensitivity in a low background environment. Measurements at the University of Notre Dame pursue a determination of the non-resonant cross section at higher energies. We present the two experiments and the status of the data analysis.
© The Authors, published by EDP Sciences, 2017
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. (http://creativecommons.org/licenses/by/4.0/).
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