6533b855fe1ef96bd12b115c

RESEARCH PRODUCT

Enhanced Quadrupole and Octupole Strength in Doubly Magic Sn132

Marc HuyseKarl JohnstonDaniel CoxDaniel CoxP. ReiterA. VogtM L Lozano BenitoJ. OjalaJ. OjalaA. BlazhevL. KayaJoakim CederkällJose RodriguezH. NaïdjaH. NaïdjaTomoaki TogashiM. SeidlitzB. SiebeckT. BerryA. IllanaK. O. ZellN. WarrC. HenrichF. WenanderJanne PakarinenJanne PakarinenF. NowackiF. NowackiM. QueiserH. De WitteJ. SnällLiam GaffneyE. SieslingHie-isolde CollaborationsD. RosiakYusuke TsunodaMaría José García BorgeMiniballG. RainovskiK. ArnswaldGianluca ColòP. Van DuppenM. Von SchmidTakaharu OtsukaR. HirschTh. Kröll

subject

PhysicsLarge Hadron Collider010308 nuclear & particles physicsProjectileMonte Carlo methodGeneral Physics and AstronomyCoulomb excitation01 natural sciencesIonExcited state0103 physical sciencesQuadrupoleAtomic physicsNuclear Experiment010306 general physicsNucleon

description

The first 2+ and 3- states of the doubly magic nucleus Sn132 are populated via safe Coulomb excitation employing the recently commissioned HIE-ISOLDE accelerator at CERN in conjunction with the highly efficient MINIBALL array. The Sn132 ions are accelerated to an energy of 5.49 MeV/nucleon and impinged on a Pb206 target. Deexciting γ rays from the low-lying excited states of the target and the projectile are recorded in coincidence with scattered particles. The reduced transition strengths are determined for the transitions 0g.s.+→21+, 0g.s.+→31-, and 21+→31- in Sn132. The results on these states provide crucial information on cross-shell configurations which are determined within large-scale shell-model and Monte Carlo shell-model calculations as well as from random-phase approximation and relativistic random-phase approximation. The locally enhanced B(E2;0g.s.+→21+) strength is consistent with the microscopic description of the structure of the respective states within all theoretical approaches. The presented results of experiment and theory can be considered to be the first direct verification of the sphericity and double magicity of Sn132. (Less)

https://doi.org/10.1103/physrevlett.121.252501