G. Zhang , M. Polettini , D. Mengoni , G. Benzoni , Z. Huang , M. Górska , A. Blazhev , L.M. Fraile , A. Gargano , G. De Gregorio , F. Nowacki , G. Aggez , U. Ahmed , O. Aktas , M. Al-Aqeel , B. Alayed , H.M. Albers , A. Algora , S. Alhomaidhi , F. Amjad , A. Zyriliou
{"title":"Approaching 100Sn: Structural evolution in 98,100Cd via lifetime measurements","authors":"G. Zhang , M. Polettini , D. Mengoni , G. Benzoni , Z. Huang , M. Górska , A. Blazhev , L.M. Fraile , A. Gargano , G. De Gregorio , F. Nowacki , G. Aggez , U. Ahmed , O. Aktas , M. Al-Aqeel , B. Alayed , H.M. Albers , A. Algora , S. Alhomaidhi , F. Amjad , A. Zyriliou","doi":"10.1016/j.physletb.2025.139378","DOIUrl":null,"url":null,"abstract":"<div><div>The lifetimes of low-lying excited states below the <span><math><msup><mrow><mn>8</mn></mrow><mrow><mo>+</mo></mrow></msup></math></span> seniority isomer were directly measured using fast timing detectors in the neutron-deficient isotopes <sup>98,100</sup>Cd. This experiment was conducted with the DEcay SPECtroscopy (DESPEC) setup at GSI, where the ions of interest were produced via a fragmentation reaction and identified using the FRagment Separator (FRS) before being implanted in the AIDA active stopper system, and the <em>γ</em> rays emitted during the de-excitation of isomeric states were detected by the LaBr<sub>3</sub> FATIMA Array. The newly deduced values for the reduced transition probabilities were compared with shell-model calculations using different interactions and effective charges. The results indicate that, while <sup>98</sup>Cd aligns well with a seniority scheme description, in <sup>100</sup>Cd the transition strengths among low-lying states are not fully reproduced, and the nature of these states remains an open problem within the present theoretical description. Ultimately, a key element in the description of this region, crucial for nuclear physics and astrophysics, appears to be the proton-neutron term of the nuclear effective interaction.</div></div>","PeriodicalId":20162,"journal":{"name":"Physics Letters B","volume":"863 ","pages":"Article 139378"},"PeriodicalIF":4.5000,"publicationDate":"2025-03-07","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/S0370269325001388","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}
引用次数: 0
Abstract
The lifetimes of low-lying excited states below the seniority isomer were directly measured using fast timing detectors in the neutron-deficient isotopes 98,100Cd. This experiment was conducted with the DEcay SPECtroscopy (DESPEC) setup at GSI, where the ions of interest were produced via a fragmentation reaction and identified using the FRagment Separator (FRS) before being implanted in the AIDA active stopper system, and the γ rays emitted during the de-excitation of isomeric states were detected by the LaBr3 FATIMA Array. The newly deduced values for the reduced transition probabilities were compared with shell-model calculations using different interactions and effective charges. The results indicate that, while 98Cd aligns well with a seniority scheme description, in 100Cd the transition strengths among low-lying states are not fully reproduced, and the nature of these states remains an open problem within the present theoretical description. Ultimately, a key element in the description of this region, crucial for nuclear physics and astrophysics, appears to be the proton-neutron term of the nuclear effective interaction.
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.