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New sub-mu s isomers in Sn-125,Sn-127,Sn-129 and isomer systematics of Sn124-130

机译:Sn-125,Sn-127,Sn-129中的新亚微米异构体和Sn124-130的异构体系统

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摘要

New sub-mu s isomers have been observed in the neutron-rich Sn isotopes. Sn-125,Sn-127,Sn-129 nuclei have been produced in a relativistic fission reaction of U-238 on a Be-9 target at 750 A.MeV and by the fragmentation of Xe-136 at 600 A.MeV populating high-spin yrast states. In addition to the already known mu s isomers, three new ones with sub-mu s half-lives have been observed. These yrast isomers are the high-spin members of the nu(d(3/2)(-1)h(11/2)(-2)) and nu h(11/2)(-n), seniority v = 3 multiplets leading to isomeric (23/2(+)) and (27/2(-)) states, respectively. Added to the already known 19/2(+)mu s isomers in this region the current work completes the systematic information of neutron-hole excitations toward the filling of the last h(11/2) orbital at N = 82. The results are discussed in the framework of state-of-the-art shell-model calculations using realistic interactions.
机译:在富含中子的锡同位素中发现了新的亚μs异构体。 Sn-125,Sn-127,Sn-129核是通过U-238在750 A.MeV上对Be-9靶标的相对论裂变反应以及在600 A.MeV上Xe-136的裂解产生的-旋转的yrast状态。除了已知的mus异构体外,还发现了三个新的具有亚μs半衰期的异构体。这些yrast异构体是nu(d(3/2)(-1)h(11/2)(-2))和nu h(11/2)(-n)的高自旋成员,资历v = 3多重态分别导致异构(23/2(+))和(27/2(-))状态。除此区域已知的19/2(+)μs异构体外,当前工作还完成了N = 82处最后一个h(11/2)轨道填充的中子-空穴激发的系统信息。在使用实际交互的最新壳模型计算框架中进行了讨论。

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