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Asymptotic normalization coefficient for 12C+p→13N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$\end{document} from the 12C(10B,9Be)13N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$\end{document} reaction and the 12C(p,γ)13N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$\end{document} astrophysical S factor

Authors
  • Artemov, S. V.1
  • Yarmukhamedov, R.1
  • Burtebayev, N.2, 3
  • Karakozov, B. K.2
  • Ergashev, F. Kh.1
  • Nassurlla, Maulen2, 3
  • Igamov, S. B.1, 4
  • Amangeldi, N.2, 5
  • Morzabayev, A.2, 5
  • Burtebayeva, J.2
  • Zhdanov, V. S.2
  • Yergaliuly, G.2, 5
  • Piasecki, E.6
  • Rusek, K.6
  • Sakuta, S. B.2, 7
  • Demyanova, A.2, 7
  • Tojiboev, O. R.1
  • Trzcińska, A.6
  • Sabidolda, A.2, 3
  • Khojayev, R.2, 3
  • And 5 more
  • 1 Institute of Nuclear Physics, Tashkent, 100214, Uzbekistan , Tashkent (Uzbekistan)
  • 2 Institute of Nuclear Physics, Almaty, 050032, Kazakhstan , Almaty (Kazakhstan)
  • 3 Al-Farabi Kazakh National University, Almaty, 050040, Kazakhstan , Almaty (Kazakhstan)
  • 4 Branch of National Research Nuclear University MEPhI, Tashkent, 100214, Uzbekistan , Tashkent (Uzbekistan)
  • 5 L.N. Gumilyov Eurasian National University, Nur-Sultan, 010008, Kazakhstan , Nur-Sultan (Kazakhstan)
  • 6 Heavy Ion Laboratory University of Warsaw, Warsaw, PL-20-093, Poland , Warsaw (Poland)
  • 7 National Research Center “Kurchatov Institute”, Moscow, 123182, Russia , Moscow (Russia)
  • 8 Gulistan State University, Gulistan, 120100, Uzbekistan , Gulistan (Uzbekistan)
  • 9 Satbayev University, Institute of Physics and Technology, Almaty, 050032, Kazakhstan , Almaty (Kazakhstan)
Type
Published Article
Journal
The European Physical Journal A
Publisher
Springer Berlin Heidelberg
Publication Date
Feb 09, 2022
Volume
58
Issue
2
Identifiers
DOI: 10.1140/epja/s10050-021-00652-z
Source
Springer Nature
Disciplines
  • Regular Article - Experimental Physics
License
Yellow

Abstract

This work is aimed at clarifying the contribution of the proton direct radiative capture to the 12C(p,γ)13N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$\end{document} reaction by specifying the value of the asymptotic normalization coefficient (ANC) for 12C+p→13Ng.s.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}\mathrm{C}+p\rightarrow {}^{13}\mathrm{N}_\mathrm{g.s.}$$\end{document}. In order to do this, the differential cross section of the proton transfer in the 12C(10B,9Be)13N\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}\mathrm{C}({}^{10}\mathrm{B},{}^9\mathrm{Be})^{13}\mathrm{N}$$\end{document} reaction at an energy of 41.3 MeV has been measured and analyzed through the modified distorted wave Born approximation (MDWBA) method taking into account the reaction channel coupling and 3He\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{3}{\mathrm{He}}$$\end{document} cluster transfer contributions. The value of the ANC was derived to be 1.63±0.13 fm-1/2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{-1/2}$$\end{document}, which was used in estimating the astrophysical S(E) factor and the reaction rate of the proton radiative capture by the 12C\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{12}{\mathrm{C}}$$\end{document} nucleus at energies of astrophysical relevance.

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