{"title":"Entrance channel-dependent compound nucleus formation probability of heavy nuclei","authors":"H S Anushree, S Shubha, H C Manjunatha, N Sowmya","doi":"10.1007/s12043-025-02900-z","DOIUrl":null,"url":null,"abstract":"<div><p>Compound nucleus (CN) formation probability (<span>\\(P_{\\textrm{CN}}\\)</span>) is essential for synthesising superheavy elements (SHEs), understanding nuclear reactions, predicting reaction outcomes and designing efficient experiments. High <span>\\(P_{\\textrm{CN}}\\)</span> indicates a greater likelihood of successful fusion, aiding in the study of nuclear stability and structure. An empirical formula for <span>\\(P_{\\textrm{CN}}\\)</span> has been proposed, incorporating new parameters such as effective fissility (<span>\\(\\chi _{\\textrm{eff}}\\)</span>) and zeta parameter (<span>\\(\\zeta \\)</span>), along with excitation energy and fusion barrier height. The fitted function shows greater systematic behaviour for <span>\\((E^*-V_B)\\chi _{\\textrm{eff}}\\)</span> and <span>\\(\\zeta ^{0.02}\\)</span>. <span>\\(P_{\\textrm{CN}}\\)</span> values obtained align well with the experimental data, predicting outcomes for both successful and unsuccessful fusion reactions. Notably, larger <span>\\(P_{\\textrm{CN}}\\)</span> values are seen for <span>\\(\\phantom {a}^{45}\\hbox {Sc}{+}^{249}\\hbox {Cf}\\)</span> and <span>\\(\\phantom {a}^{50}\\hbox {Ti}{+}^{249}\\hbox {Bk}\\)</span> for <span>\\(Z=119\\)</span> and 120, respectively. Analysis identifies <span>\\(\\phantom {a}^{80}\\hbox {Se}{+}^{210}\\hbox {At}\\)</span> and <span>\\(\\phantom {a}^{55}\\hbox {Mn}{+}^{241}\\hbox {Pu}\\)</span> as potential reactions for synthesising the SHE (<span>\\(Z=119\\)</span>), with Mn projectiles showing higher <span>\\(P_{\\textrm{CN}}\\)</span> than Se projectiles due to lower <span>\\(\\zeta \\)</span> and deformation effects. Hence, <span>\\(\\phantom {a}^{55}\\hbox {Mn}{+}^{241}\\hbox {Pu}\\)</span> is more promising than <span>\\(\\phantom {a}^{80}\\hbox {Se}{+}^{210}\\hbox {At}\\)</span> for this purpose. The present work is useful for focussing experimental efforts and increasing the efficiency of SHE research by focussing on reactions with higher CN formation probability.</p></div>","PeriodicalId":743,"journal":{"name":"Pramana","volume":"99 2","pages":""},"PeriodicalIF":1.9000,"publicationDate":"2025-03-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Pramana","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1007/s12043-025-02900-z","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
Compound nucleus (CN) formation probability (\(P_{\textrm{CN}}\)) is essential for synthesising superheavy elements (SHEs), understanding nuclear reactions, predicting reaction outcomes and designing efficient experiments. High \(P_{\textrm{CN}}\) indicates a greater likelihood of successful fusion, aiding in the study of nuclear stability and structure. An empirical formula for \(P_{\textrm{CN}}\) has been proposed, incorporating new parameters such as effective fissility (\(\chi _{\textrm{eff}}\)) and zeta parameter (\(\zeta \)), along with excitation energy and fusion barrier height. The fitted function shows greater systematic behaviour for \((E^*-V_B)\chi _{\textrm{eff}}\) and \(\zeta ^{0.02}\). \(P_{\textrm{CN}}\) values obtained align well with the experimental data, predicting outcomes for both successful and unsuccessful fusion reactions. Notably, larger \(P_{\textrm{CN}}\) values are seen for \(\phantom {a}^{45}\hbox {Sc}{+}^{249}\hbox {Cf}\) and \(\phantom {a}^{50}\hbox {Ti}{+}^{249}\hbox {Bk}\) for \(Z=119\) and 120, respectively. Analysis identifies \(\phantom {a}^{80}\hbox {Se}{+}^{210}\hbox {At}\) and \(\phantom {a}^{55}\hbox {Mn}{+}^{241}\hbox {Pu}\) as potential reactions for synthesising the SHE (\(Z=119\)), with Mn projectiles showing higher \(P_{\textrm{CN}}\) than Se projectiles due to lower \(\zeta \) and deformation effects. Hence, \(\phantom {a}^{55}\hbox {Mn}{+}^{241}\hbox {Pu}\) is more promising than \(\phantom {a}^{80}\hbox {Se}{+}^{210}\hbox {At}\) for this purpose. The present work is useful for focussing experimental efforts and increasing the efficiency of SHE research by focussing on reactions with higher CN formation probability.
期刊介绍:
Pramana - Journal of Physics is a monthly research journal in English published by the Indian Academy of Sciences in collaboration with Indian National Science Academy and Indian Physics Association. The journal publishes refereed papers covering current research in Physics, both original contributions - research papers, brief reports or rapid communications - and invited reviews. Pramana also publishes special issues devoted to advances in specific areas of Physics and proceedings of select high quality conferences.