EPJ Web Conf.
Volume 227, 202010th European Summer School on Experimental Nuclear Astrophysics
|Number of page(s)||4|
|Section||Session 2: Contribution by Young Researchers|
|Published online||14 January 2020|
Study of the 22Ne(α , γ)26Mg reaction at LUNA
1 Universitk degli studi di Milano and INFN, Sezione di Milano, Milano, Italy
* e-mail: firstname.lastname@example.org
Published online: 14 January 2020
The 22Ne( α , γ)26Mg reaction competes with the 22Ne(α, n)25Mg reac-tion which is the main source of neutrons for the s-process in low-mass Asymptotic Giant Branch (AGB) and massive stars. The 22Ne( α , γ)26Mg reaction rateis affected by a high uncertainty mainly due to the poorly constrained 395 keVresonance which has been studied only indirectly leading to a wide range of pos-sible values for its resonance strength (10-14 - 10-9 eV). The present study represents the direct measurement of the 395 keV resonance of the 22Ne( α , γ)26Mgreaction at LUNA (Laboratory for Underground Nuclear Astrophysics), located at Gran Sasso National Laboratory. Here, the experimental campaigns, setupand some very preliminary results are presented.
© The Authors, published by EDP Sciences, 2020
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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