Nuclear clustering—manifestations of non-uniformity in nuclei

Author:

Uesaka T.123ORCID,Itagaki N.145ORCID

Affiliation:

1. RIKEN Nishina Center for Accelerator-Based Science , Saitama 351-0198, Japan

2. RIKEN Cluster for Pioneering Research , Saitama 351-0198, Japan

3. Graduate School of Science and Engineering, Saitama University , Saitama 338-8570, Japan

4. Department of Physics, Osaka Metropolitan University , Osaka 558-8585, Japan

5. Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP), Osaka Metropolitan University , Osaka 558-8585, Japan

Abstract

Well-developed α clusters are known to exist in light N = Z nuclei, and their properties are reasonably well described with modern nuclear structure theories. However, ‘modestly’ developed clusters in medium to heavy nuclei remain little understood, both theoretically and experimentally. Extension of the focus to include modestly developed clusters leads us to a concept of ‘generalized clusters’ and ‘cluster ubiquitousness’. The former includes clusters more weakly bound than an α cluster, such as deuteron, triton and He 3 , and even clusters partially broken owing to nuclear medium effects. The latter means the existence of clusters in any nuclei, where cluster development was not previously discussed. Effects of the tensor and the spin–orbit interactions on the coexistence of clusters with independent nucleons are discussed using recent nuclear theoretical models. A mixture of the clusters with shell-like components plays an essential role in the synthesis of elements in the universe and the origin of life, together with an α decay. It is also pointed out that clustering in heavy nuclei may accelerate fission and fusion processes. Future experimental plans using cluster knockout reactions, which have the potential to extract information of ‘generalized clusters’ in a variety of nuclei including stable and unstable nuclei, are also discussed. This article is part of the theme issue ‘The liminal position of Nuclear Physics: from hadrons to neutron stars’.

Funder

Japan Society for the Promotion of Science

Publisher

The Royal Society

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