S.K. Sakhiyev , S.V. Artemov , N. Burtebayev , S.B. Sakuta , S.B. Igamov , Maulen Nassurlla , K. Rusek , M. Wolińska-Cichocka , N. Amangeldi , Marzhan Nassurlla , A. Trzcińska , G. Yergaliuly , F.Kh. Ergashev , O.R. Tojiboev , I.Ya. Son , A. Sabidolda , R. Khojayev , Y.B. Mukanov , D.A. Issayev
{"title":"Asymptotic normalization coefficients for 11B + p → 12C from the 11B(10B, 9Be)12C reaction and the 11B(p, γ)12C astrophysical S-factor","authors":"S.K. Sakhiyev , S.V. Artemov , N. Burtebayev , S.B. Sakuta , S.B. Igamov , Maulen Nassurlla , K. Rusek , M. Wolińska-Cichocka , N. Amangeldi , Marzhan Nassurlla , A. Trzcińska , G. Yergaliuly , F.Kh. Ergashev , O.R. Tojiboev , I.Ya. Son , A. Sabidolda , R. Khojayev , Y.B. Mukanov , D.A. Issayev","doi":"10.1016/j.rinp.2024.108050","DOIUrl":null,"url":null,"abstract":"<div><div>The <sup>11</sup>B(<sup>10</sup>B,<sup>9</sup>Be)<sup>12</sup>C reaction was studied at the energy of 41.3 MeV with transitions to the ground (0<sup>+</sup>) and low-lying excited 4.44 MeV (2<sup>+</sup>) and 9.64 MeV (3<sup>−</sup>) states of <sup>12</sup>C nucleus. The analysis of the measured angular distributions was carried out using a modified distorted wave (MDWBA) method, assuming a one-step proton transfer mechanism. It was shown that at small angles (in the region of the main diffraction maximum) this reaction occurs on the nuclear surface with the dominance of a one-step process. This made possible to determine the values of asymptotic normalization coefficients (ANC) for <sup>11</sup>B + <em>p</em> → <sup>12</sup>C. The squared ANCs equal to 322 ± 76 fm<sup>−1</sup>, 32.8 ± 8.4 fm<sup>−1</sup> and 1.26 ± 0.44 fm<sup>−1</sup> for 0<sup>+</sup>, 2<sup>+</sup> and 3<sup>−</sup> states of the <sup>12</sup>C nucleus respectively were obtained. These values were used to take into account the contribution of the direct process in the calculation of astrophysical <em>S</em>-factors for the radiative capture of a proton by the <sup>11</sup>B nucleus at astrophysical energies.</div></div>","PeriodicalId":21042,"journal":{"name":"Results in Physics","volume":"67 ","pages":"Article 108050"},"PeriodicalIF":4.4000,"publicationDate":"2024-11-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Results in Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2211379724007356","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"MATERIALS SCIENCE, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
The 11B(10B,9Be)12C reaction was studied at the energy of 41.3 MeV with transitions to the ground (0+) and low-lying excited 4.44 MeV (2+) and 9.64 MeV (3−) states of 12C nucleus. The analysis of the measured angular distributions was carried out using a modified distorted wave (MDWBA) method, assuming a one-step proton transfer mechanism. It was shown that at small angles (in the region of the main diffraction maximum) this reaction occurs on the nuclear surface with the dominance of a one-step process. This made possible to determine the values of asymptotic normalization coefficients (ANC) for 11B + p → 12C. The squared ANCs equal to 322 ± 76 fm−1, 32.8 ± 8.4 fm−1 and 1.26 ± 0.44 fm−1 for 0+, 2+ and 3− states of the 12C nucleus respectively were obtained. These values were used to take into account the contribution of the direct process in the calculation of astrophysical S-factors for the radiative capture of a proton by the 11B nucleus at astrophysical energies.
Results in PhysicsMATERIALS SCIENCE, MULTIDISCIPLINARYPHYSIC-PHYSICS, MULTIDISCIPLINARY
CiteScore
8.70
自引率
9.40%
发文量
754
审稿时长
50 days
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