Numerical study of transition rate and B(E2) transition strengths for <superscript>17</superscript>O(p,γ) <superscript>18</superscript>F reaction. (English)
In: Journal of Research on Many-Body Systems, Jg. 13 (2024), Heft 4, S. 29-40
academicJournal
Zugriff:
The study of the astrophysical S-factor is one of the methods of analyzing proton radiation capture reactions in the theoretical framework for low temperatures. In this research, we have numerically studied the proton radiative capture reaction by 17O using the Woods-Saxon potential model. First, the astrophysical S-factor 17 O(p,γ) 18 F reaction was calculated at low energies, and then the reaction rate of 17 O(p,γ) 18 F was obtained from the astrophysical S-factor. Also, in this study, the electrical quadrupole transition strength (B[E2]) for excited states 18 F nucleus has been calculated. We found that B[E2] depends on the energy and spin of the excited states. The results corresponding to the astrophysical S-factor, reaction rate and transition strength at energy range of 200-500 keV were compared with experimental data and other theoretical models and were in good agreement. Also, the astrophysical S-factor at zero energy was calculated by the extrapolation method for (5/2) + state and S(0)=4/8 keV b. [ABSTRACT FROM AUTHOR]
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Titel: |
Numerical study of transition rate and B(E2) transition strengths for <superscript>17</superscript>O(p,γ) <superscript>18</superscript>F reaction. (English)
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Autor/in / Beteiligte Person: | Aranpour, Amir Hooman ; Khalili, Hasan ; Nahidinezhad, Shahla ; Dalvand, Maasoumeh |
Zeitschrift: | Journal of Research on Many-Body Systems, Jg. 13 (2024), Heft 4, S. 29-40 |
Veröffentlichung: | 2024 |
Medientyp: | academicJournal |
ISSN: | 2322-231X (print) |
DOI: | 10.22055/jrmbs.2024.18898 |
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