Chapter III. Study of Non-Alpha-Nuclei Based on the Viewpoint of Cluster Correlations
Hiroshi Furutani,Hiroyuki Kanada,Tsuneo Kaneko,Sinobu Nagata,Hidetoshi Nishioka,Shigeto Okabe,Sakae Saito,Toshimi Sakuda,Michio Seya +8 more
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This article is published in Progress of Theoretical Physics Supplement.The article was published on 1980-01-01 and is currently open access. It has received 79 citations till now. The article focuses on the topics: Cluster (physics).read more
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The clustered nucleus—cluster structures in stable and unstable nuclei
TL;DR: In this paper, a review of the development of clustering in light nuclei is presented, mostly from the stand-point of the harmonic oscillator framework, which allows a unifying description of alpha-conjugate and neutron-rich nuclei.
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Recent development of complex scaling method for many-body resonances and continua in light nuclei
TL;DR: The complex scaling method (CSM) as mentioned in this paper is a useful similarity transformation of the Schrodinger equation, in which bound-state spectra are not changed but continuum spectra can be separated into resonant and non-resonant ones.
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Developments in the study of nuclear clustering in light even - even nuclei
M. Freer,A C Merchant +1 more
TL;DR: In this paper, the role of clustering and cluster models in nuclear reactions is investigated and a review of the developments in the experimental and theoretical understanding of cluster symmetries is presented.
Journal ArticleDOI
Recent development of complex scaling method for many-body resonances and continua in light nuclei
TL;DR: The complex scaling method (CSM) as discussed by the authors is a useful similarity transformation of the Schrodinger equation, in which bound-state spectra are not changed but continuum spectras are separated into resonant and non-resonant continuum ones.
Journal ArticleDOI
Stellar Production Rates of Carbon and Its Abundance in the Universe
TL;DR: It is shown that outside a narrow window of 0.5 and 4% of the values of the strong and Coulomb forces, respectively, the stellar production of carbon or oxygen is reduced by factors of 30 to 1000.