F.R. Vasconcelos, G.F.D. Abreu, E.N. Cardozo, J. Lubian
{"title":"Nuclear mass density effect of 27Al and 28Si nuclei in nuclear reactions","authors":"F.R. Vasconcelos, G.F.D. Abreu, E.N. Cardozo, J. Lubian","doi":"10.1016/j.nuclphysa.2025.123240","DOIUrl":null,"url":null,"abstract":"<div><div>In a recent study, diffuseness parameters of <span><math><mrow><msub><mi>a</mi><mi>m</mi></msub><mo>=</mo><mn>0.62</mn><mspace></mspace><mrow><mi>fm</mi></mrow></mrow></math></span> and <span><math><mrow><msub><mi>a</mi><mi>m</mi></msub><mo>=</mo><mn>0.65</mn><mspace></mspace><mrow><mi>fm</mi></mrow></mrow></math></span> were proposed for the nuclear matter density of <span><math><msup><mrow></mrow><mn>28</mn></msup></math></span>Si and <span><math><msup><mrow></mrow><mn>27</mn></msup></math></span>Al, respectively, based on the two-parameter Fermi distribution. These values exceed the systematic value <span><math><mrow><msub><mi>a</mi><mi>m</mi></msub><mo>=</mo><mn>0.56</mn><mspace></mspace><mrow><mi>fm</mi></mrow></mrow></math></span>, commonly adopted in the São Paulo potential. To assess the validity of the proposed parameters, we performed coupled-channel calculations for the systems <span><math><msup><mrow></mrow><mn>9</mn></msup></math></span>Be+<span><math><msup><mrow></mrow><mn>28</mn></msup></math></span>Si, <span><math><msup><mrow></mrow><mn>14</mn></msup></math></span>N+<span><math><msup><mrow></mrow><mn>28</mn></msup></math></span>Si, <span><math><msup><mrow></mrow><mn>13</mn></msup></math></span>C+<span><math><msup><mrow></mrow><mn>28</mn></msup></math></span>Si, <span><math><msup><mrow></mrow><mn>9</mn></msup></math></span>Be+<span><math><msup><mrow></mrow><mn>27</mn></msup></math></span>Al, <span><math><msup><mrow></mrow><mn>14</mn></msup></math></span>N+<span><math><msup><mrow></mrow><mn>27</mn></msup></math></span>Al, and <span><math><msup><mrow></mrow><mn>28</mn></msup></math></span>Si+<span><math><msup><mrow></mrow><mn>27</mn></msup></math></span>Al at energies 2-3 times the Coulomb barrier. The analyses were carried out using the FRESCO code, with the Sao Paulo Potential and Woods-Saxon potential used as the optical potential. A good description of elastic angular distributions was achieved with the systematic nuclear matter density diffuseness value of <span><math><mrow><msub><mi>a</mi><mi>m</mi></msub><mo>=</mo><mn>0.56</mn><mspace></mspace><mrow><mi>fm</mi></mrow></mrow></math></span>.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1064 ","pages":"Article 123240"},"PeriodicalIF":2.5000,"publicationDate":"2025-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear Physics A","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S037594742500226X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, NUCLEAR","Score":null,"Total":0}
引用次数: 0
Abstract
In a recent study, diffuseness parameters of and were proposed for the nuclear matter density of Si and Al, respectively, based on the two-parameter Fermi distribution. These values exceed the systematic value , commonly adopted in the São Paulo potential. To assess the validity of the proposed parameters, we performed coupled-channel calculations for the systems Be+Si, N+Si, C+Si, Be+Al, N+Al, and Si+Al at energies 2-3 times the Coulomb barrier. The analyses were carried out using the FRESCO code, with the Sao Paulo Potential and Woods-Saxon potential used as the optical potential. A good description of elastic angular distributions was achieved with the systematic nuclear matter density diffuseness value of .
期刊介绍:
Nuclear Physics A focuses on the domain of nuclear and hadronic physics and includes the following subsections: Nuclear Structure and Dynamics; Intermediate and High Energy Heavy Ion Physics; Hadronic Physics; Electromagnetic and Weak Interactions; Nuclear Astrophysics. The emphasis is on original research papers. A number of carefully selected and reviewed conference proceedings are published as an integral part of the journal.