Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor

Artemov, S. V.; Yarmukhamedov, R.; Burtebayev, N.; Karakozov, B. K.; Ergashev, F. Kh.; Nassurlla, M.; Igamov, S. B.; Amangeldi, N.; Morzabayev, A. K.; Burtebayeva, J.; Zhdanov, V. S.; Yergaliuly, G.; Piasecki, E.; Rusek, K.; Sakuta, S.B.; Demyanova, A. S.; Tojiboev, O. R.; Trzcińska, A.; Sabidolda, A.; Khojayev, R.; Tursunmakhatov, K. I.; Nassurlla, M.; Wolińska-Cichocka, M.; Sadykov, T. Kh.; Saduyev, N.

doi:10.1140/epja/s10050-021-00652-z

Eur. Phys. J. A

2022

DOI: 10.1140/epja/s10050-021-00652-z

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Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor

S. V. Artemov

R. Yarmukhamedov

N. Burtebayev

et al.

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Cited by 8 publications

References 48 publications

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Clusters in light nuclei: history and recent developments

Lombardo,

Dell’Aquila

2023

Riv. Nuovo Cim.

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In this review, we discuss recent advancements in the study of clustering phenomena occurring in light nuclei, and their influence on nuclear structure, dynamics, and astrophysics. In the introduction, we outline the historical steps leading to the concept of $$\alpha $$ α -clusterization in nuclei and provide a comprehensive description of the evolution of nuclear models capable to describe clustering aspects in nuclear systems and of the main experiments and discoveries leading to the development of this research field. We also describe some spectroscopic techniques that are used to establish the clustered nature of a given nuclear state. Some relevant experimental and theoretical findings recently reported both in experimental and theoretical works are discussed in the text. We put emphasis on recent achievements and remaining problems in the description of the structure of light isotopes, from helium to neon, including both self- and non-self-conjugate nuclei. Particular attention to the implication in the nuclear astrophysics context and to clustering effects in the dynamics of nuclear reactions is pursued all along the review.

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Clusters in light nuclei: history and recent developments

Lombardo,

Dell’Aquila

2023

Riv. Nuovo Cim.

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Energy Levels of Light Nuclei A=13

Kelley,

Sheu,

Purcell

2024

Nuclear Data Sheets

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Precise resonance parameter measurement in the 12C(p,γ)13N astrophysically important reaction

2023

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Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor

Cited by 8 publications

References 48 publications

Clusters in light nuclei: history and recent developments

Clusters in light nuclei: history and recent developments

Energy Levels of Light Nuclei A=13

Precise resonance parameter measurement in the 12C(p,γ)13N astrophysically important reaction

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