{"title":"对 Li6 与 H3 和 He3 核相互作用所引发反应的理论分析","authors":"Yu. A. Lashko, V. S. Vasilevsky, V. I. Zhaba","doi":"10.1103/physrevc.110.035806","DOIUrl":null,"url":null,"abstract":"We determine cross sections and astrophysical <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>S</mi></math> factors of the reactions generated in collisions between <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi mathvariant=\"normal\">H</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> and between <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>He</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math>. A microscopic three-cluster model is employed to study the dynamics of reactions occurring in the mirror nuclei <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi mathvariant=\"normal\">B</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math>. In a previous study [<span>Phys. Rev. C</span> <b>109</b>, 045803 (2024)], this model was successfully applied to investigate the resonance structure of <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi mathvariant=\"normal\">B</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math>, as well as reactions induced by the interaction of deuterons with <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>7</mn></mmultiscripts></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>7</mn></mmultiscripts></math>. A fairly good agreement between theoretical results and available experimental data was achieved. To the best of our knowledge, appropriate experimental data for the astrophysical <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>S</mi></math> factors of the reactions generated by the interaction of <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> with <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi mathvariant=\"normal\">H</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> and with <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>He</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> are currently unavailable. Thus, our results can serve as a guideline for future experimental efforts.","PeriodicalId":20122,"journal":{"name":"Physical Review C","volume":"8 1","pages":""},"PeriodicalIF":3.1000,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Theoretical analysis of the reactions induced by interaction of Li6 with H3 and He3 nuclei\",\"authors\":\"Yu. A. Lashko, V. S. Vasilevsky, V. I. Zhaba\",\"doi\":\"10.1103/physrevc.110.035806\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We determine cross sections and astrophysical <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>S</mi></math> factors of the reactions generated in collisions between <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi mathvariant=\\\"normal\\\">H</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> and between <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>He</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math>. A microscopic three-cluster model is employed to study the dynamics of reactions occurring in the mirror nuclei <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math> and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi mathvariant=\\\"normal\\\">B</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math>. In a previous study [<span>Phys. Rev. C</span> <b>109</b>, 045803 (2024)], this model was successfully applied to investigate the resonance structure of <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math> and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi mathvariant=\\\"normal\\\">B</mi><mprescripts></mprescripts><none></none><mn>9</mn></mmultiscripts></math>, as well as reactions induced by the interaction of deuterons with <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>7</mn></mmultiscripts></math> and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Be</mi><mprescripts></mprescripts><none></none><mn>7</mn></mmultiscripts></math>. A fairly good agreement between theoretical results and available experimental data was achieved. To the best of our knowledge, appropriate experimental data for the astrophysical <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>S</mi></math> factors of the reactions generated by the interaction of <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Li</mi><mprescripts></mprescripts><none></none><mn>6</mn></mmultiscripts></math> with <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi mathvariant=\\\"normal\\\">H</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> and with <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>He</mi><mprescripts></mprescripts><none></none><mn>3</mn></mmultiscripts></math> are currently unavailable. Thus, our results can serve as a guideline for future experimental efforts.\",\"PeriodicalId\":20122,\"journal\":{\"name\":\"Physical Review C\",\"volume\":\"8 1\",\"pages\":\"\"},\"PeriodicalIF\":3.1000,\"publicationDate\":\"2024-09-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical Review C\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/physrevc.110.035806\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review C","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevc.110.035806","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
Theoretical analysis of the reactions induced by interaction of Li6 with H3 and He3 nuclei
We determine cross sections and astrophysical factors of the reactions generated in collisions between and and between and . A microscopic three-cluster model is employed to study the dynamics of reactions occurring in the mirror nuclei and . In a previous study [Phys. Rev. C109, 045803 (2024)], this model was successfully applied to investigate the resonance structure of and , as well as reactions induced by the interaction of deuterons with and . A fairly good agreement between theoretical results and available experimental data was achieved. To the best of our knowledge, appropriate experimental data for the astrophysical factors of the reactions generated by the interaction of with and with are currently unavailable. Thus, our results can serve as a guideline for future experimental efforts.
期刊介绍:
Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field.
PRC covers experimental and theoretical results in all aspects of nuclear physics, including:
Nucleon-nucleon interaction, few-body systems
Nuclear structure
Nuclear reactions
Relativistic nuclear collisions
Hadronic physics and QCD
Electroweak interaction, symmetries
Nuclear astrophysics