B. Huang , F.P. Bai , J.G. Li , D.Q. Fang , S.M. Wang
{"title":"探索38,39ti可能的双质子放射性","authors":"B. Huang , F.P. Bai , J.G. Li , D.Q. Fang , S.M. Wang","doi":"10.1016/j.physletb.2025.139257","DOIUrl":null,"url":null,"abstract":"<div><div>Two-proton (2<em>p</em>) radioactivity represents a rare decay mode that has been experimentally observed only in a selected few nuclei. The exploration of 2<em>p</em> emission is crucial for elucidating the structure, mass, and nucleon-nucleon interactions within exotic proton-rich nuclei. <sup>39</sup>Ti has long been postulated as a potential candidate for 2<em>p</em> emission; however, experimental investigations have yet to confirm its 2<em>p</em> decay. To provide more accurate information for further studies, we utilize the Gamow shell model (GSM) and the Gamow coupled channel (GCC) method to analyze the prospective 2<em>p</em> radioactivity of isotopes <sup>38,39</sup>Ti. Our calculations suggest that <sup>39</sup>Ti is indeed a viable candidate for 2<em>p</em> emission. Notably, the estimated partial 2<em>p</em> decay width for <sup>39</sup>Ti, predicted from the three-body GCC method, suggests that its 2<em>p</em> decay could rival its <em>β</em> decay in likelihood, although this is highly dependent on the specific 2<em>p</em> decay energy. Additionally, our analysis indicates a propensity for pairing between the valence protons in <sup>39</sup>Ti. A similar investigative approach reveals that <sup>38</sup>Ti exhibits a higher 2<em>p</em> decay energy and a broader decay width than <sup>39</sup>Ti, positioning it as a more promising candidate for 2<em>p</em> decay.</div></div>","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"861 ","pages":"Article 139257"},"PeriodicalIF":4.3000,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Exploring the possible two-proton radioactivity of 38,39Ti\",\"authors\":\"B. Huang , F.P. Bai , J.G. Li , D.Q. Fang , S.M. Wang\",\"doi\":\"10.1016/j.physletb.2025.139257\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Two-proton (2<em>p</em>) radioactivity represents a rare decay mode that has been experimentally observed only in a selected few nuclei. The exploration of 2<em>p</em> emission is crucial for elucidating the structure, mass, and nucleon-nucleon interactions within exotic proton-rich nuclei. <sup>39</sup>Ti has long been postulated as a potential candidate for 2<em>p</em> emission; however, experimental investigations have yet to confirm its 2<em>p</em> decay. To provide more accurate information for further studies, we utilize the Gamow shell model (GSM) and the Gamow coupled channel (GCC) method to analyze the prospective 2<em>p</em> radioactivity of isotopes <sup>38,39</sup>Ti. Our calculations suggest that <sup>39</sup>Ti is indeed a viable candidate for 2<em>p</em> emission. Notably, the estimated partial 2<em>p</em> decay width for <sup>39</sup>Ti, predicted from the three-body GCC method, suggests that its 2<em>p</em> decay could rival its <em>β</em> decay in likelihood, although this is highly dependent on the specific 2<em>p</em> decay energy. Additionally, our analysis indicates a propensity for pairing between the valence protons in <sup>39</sup>Ti. A similar investigative approach reveals that <sup>38</sup>Ti exhibits a higher 2<em>p</em> decay energy and a broader decay width than <sup>39</sup>Ti, positioning it as a more promising candidate for 2<em>p</em> decay.</div></div>\",\"PeriodicalId\":20162,\"journal\":{\"name\":\"Physics Letters B\",\"volume\":\"861 \",\"pages\":\"Article 139257\"},\"PeriodicalIF\":4.3000,\"publicationDate\":\"2025-02-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics Letters B\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0370269325000176\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Letters B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0370269325000176","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Exploring the possible two-proton radioactivity of 38,39Ti
Two-proton (2p) radioactivity represents a rare decay mode that has been experimentally observed only in a selected few nuclei. The exploration of 2p emission is crucial for elucidating the structure, mass, and nucleon-nucleon interactions within exotic proton-rich nuclei. 39Ti has long been postulated as a potential candidate for 2p emission; however, experimental investigations have yet to confirm its 2p decay. To provide more accurate information for further studies, we utilize the Gamow shell model (GSM) and the Gamow coupled channel (GCC) method to analyze the prospective 2p radioactivity of isotopes 38,39Ti. Our calculations suggest that 39Ti is indeed a viable candidate for 2p emission. Notably, the estimated partial 2p decay width for 39Ti, predicted from the three-body GCC method, suggests that its 2p decay could rival its β decay in likelihood, although this is highly dependent on the specific 2p decay energy. Additionally, our analysis indicates a propensity for pairing between the valence protons in 39Ti. A similar investigative approach reveals that 38Ti exhibits a higher 2p decay energy and a broader decay width than 39Ti, positioning it as a more promising candidate for 2p decay.
期刊介绍:
Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.