https://doi.org/10.1140/epja/s10050-024-01305-7
Regular Article - Theoretical Physics
Alpha-like correlations in 20Ne, comparison of quartetting wave function and THSR approaches
1
Institut für Physik, Universität Rostock, 18051, Rostock, Germany
2
School of Physics, Nanjing University, 210093, Nanjing, China
3
Key Laboratory of Nuclear Physics and Ion-Beam Application (MoE), Institute of Modern Physics, Fudan University, 200433, Shanghai, China
4
Shanghai Research Center for Theoretical Nuclear Physics, NSFC and Fudan University, 200438, Shanghai, China
5
School of Physics Science and Engineering, Tongji University, 200092, Shanghai, China
6
Laboratory of Physics, Kanto Gakuin University, 236-8501, Yokohama, Japan
7
Research Center for Nuclear Physics (RCNP), Osaka University, 567-0047, Osaka, Japan
8
College of Science, Nanjing University of Aeronautics and Astronautics, Nanjing, China
Received:
9
February
2024
Accepted:
18
March
2024
Published online:
17
April
2024
Ne can be considered as a double-magic O core nucleus surrounded by four nucleons, the constituents of an -like quartet. Similar to other nuclei (Po, Ti, etc.) with a quartet on top of a double-magic core nucleus, significant -like correlations are expected. Correlations in the ground state of Ne are investigated using different approaches. The quartetting wave function approach (QWFA) predicts a large -like cluster contribution near the surface of the nuclei. The Tohsaki-Horiuchi-Schuck-Röpke (THSR) approach describes -like clustering in nuclear systems. The results of the QWFA in the Thomas-Fermi and shell-model approximation are compared with THSR calculations for the container model. Results for the formation probability and the rms radii are shown.
© The Author(s) 2024
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.