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核聚集——细胞核不均匀性的表现

Nuclear clustering-manifestations of non-uniformity in nuclei.

作者信息

Uesaka T, Itagaki N

机构信息

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

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

出版信息

Philos Trans A Math Phys Eng Sci. 2024 Jul 23;382(2275):20230123. doi: 10.1098/rsta.2023.0123. Epub 2024 Jun 24.

DOI:10.1098/rsta.2023.0123
PMID:38910397
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11343306/
Abstract

Well-developed [Formula: see text] clusters are known to exist in light [Formula: see text] 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 [Formula: see text] cluster, such as deuteron, triton and [Formula: see text], 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 [Formula: see text] 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'.

摘要

众所周知,在轻[公式:见正文]核中存在发育良好的[公式:见正文]集团,并且现代核结构理论能够较为合理地描述它们的性质。然而,对于中重核中“适度”发育的集团,在理论和实验方面仍知之甚少。将研究重点扩展到包括适度发育的集团,这使我们引出了“广义集团”和“集团普遍性”的概念。前者包括比[公式:见正文]集团束缚更弱的集团,如氘核、氚核和[公式:见正文],甚至包括由于核介质效应而部分破裂的集团。后者意味着在任何原子核中都存在集团,而此前并未讨论过集团的发育情况。利用最新的核理论模型,讨论了张量相互作用和自旋 - 轨道相互作用对集团与独立核子共存的影响。集团与壳层状成分的混合在宇宙中元素的合成以及生命起源中,与[公式:见正文]衰变一起起着至关重要的作用。还指出重核中的集团化可能会加速裂变和聚变过程。本文还讨论了未来使用集团敲出反应的实验计划,这种反应有可能提取包括稳定和不稳定核在内的各种原子核中“广义集团”的信息。本文是主题为“核物理的临界位置:从强子到中子星”的一部分。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/52a6d263d1b4/rsta.2023.0123.f009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/4ca5739592ab/rsta.2023.0123.f001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/00a247fd722a/rsta.2023.0123.f002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/b8209745a19b/rsta.2023.0123.f003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/b35540d2cd47/rsta.2023.0123.f004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/992ce0d2668e/rsta.2023.0123.f005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/3a2263d133b4/rsta.2023.0123.f006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/4aaf3cfd65ef/rsta.2023.0123.f007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/490e6559cb3b/rsta.2023.0123.f008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/52a6d263d1b4/rsta.2023.0123.f009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/4ca5739592ab/rsta.2023.0123.f001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/00a247fd722a/rsta.2023.0123.f002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/b8209745a19b/rsta.2023.0123.f003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/b35540d2cd47/rsta.2023.0123.f004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/992ce0d2668e/rsta.2023.0123.f005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/3a2263d133b4/rsta.2023.0123.f006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/4aaf3cfd65ef/rsta.2023.0123.f007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/490e6559cb3b/rsta.2023.0123.f008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/92ce/11343306/52a6d263d1b4/rsta.2023.0123.f009.jpg

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