{"title":"完全聚变反应的天体物理 S 因子 $$^{12,13}\\textrm{C}\\,+\\,^{12,13}$$ C","authors":"V. V. Sargsyan, G. G. Adamian, N. V. Antonenko","doi":"10.1140/epja/s10050-024-01406-3","DOIUrl":null,"url":null,"abstract":"<div><p>Comparative analysis of the complete fusion reactions <span>\\(^{12}\\textrm{C}\\, +\\, ^{12}\\textrm{C}, ^{12}\\textrm{C}\\, +\\, ^{13}\\)</span>C and <span>\\(^{13}\\textrm{C}\\, +\\, ^{13}\\)</span>C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical <i>S</i>-factor for these reactions.</p></div>","PeriodicalId":786,"journal":{"name":"The European Physical Journal A","volume":"60 9","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Astrophysical S-factors for complete fusion reactions \\\\(^{12,13}\\\\textrm{C}\\\\,+\\\\,^{12,13}\\\\)C\",\"authors\":\"V. V. Sargsyan, G. G. Adamian, N. V. Antonenko\",\"doi\":\"10.1140/epja/s10050-024-01406-3\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Comparative analysis of the complete fusion reactions <span>\\\\(^{12}\\\\textrm{C}\\\\, +\\\\, ^{12}\\\\textrm{C}, ^{12}\\\\textrm{C}\\\\, +\\\\, ^{13}\\\\)</span>C and <span>\\\\(^{13}\\\\textrm{C}\\\\, +\\\\, ^{13}\\\\)</span>C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical <i>S</i>-factor for these reactions.</p></div>\",\"PeriodicalId\":786,\"journal\":{\"name\":\"The European Physical Journal A\",\"volume\":\"60 9\",\"pages\":\"\"},\"PeriodicalIF\":2.6000,\"publicationDate\":\"2024-09-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The European Physical Journal A\",\"FirstCategoryId\":\"4\",\"ListUrlMain\":\"https://link.springer.com/article/10.1140/epja/s10050-024-01406-3\",\"RegionNum\":3,\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The European Physical Journal A","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1140/epja/s10050-024-01406-3","RegionNum":3,"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}
Astrophysical S-factors for complete fusion reactions \(^{12,13}\textrm{C}\,+\,^{12,13}\)C
Comparative analysis of the complete fusion reactions \(^{12}\textrm{C}\, +\, ^{12}\textrm{C}, ^{12}\textrm{C}\, +\, ^{13}\)C and \(^{13}\textrm{C}\, +\, ^{13}\)C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical S-factor for these reactions.
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