6533b826fe1ef96bd1283b06

RESEARCH PRODUCT

Sub-Barrier Coulomb Excitation ofSn110and Its Implications for theSn100Shell Closure

F. AmesM. Hjorth-jensenO. NiedermaierDirk SchwalmA. M. HurstU. Datta PramanikGeorgi P. GeorgievS. FranchooN. WarrHeiko ScheitP. Van DuppenT. SieberDirk WeisshaarUlli KösterP. A. ButlerFredrik WenanderJ. EberthThomas NilssonB. A. MarshB. A. MarshJoakim CederkällJoakim CederkällDietrich HabsG. SlettenMark HuyseJ. IwanickiJ. Van De WalleO. IvanovA. BanuOliver KesterThomas DavinsonClaes FahlanderAndreas EkströmI. StefanescuP. ReiterM. Górska

subject

PhysicsMass numberIsotope010308 nuclear & particles physicsShell (structure)Nuclear shell modelGeneral Physics and AstronomyCoulomb excitation7. Clean energy01 natural sciencesClosure (computer programming)Excited state0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physics

description

The first excited 2(+) state of the unstable isotope Sn-110 has been studied in safe Coulomb excitation at 2.82 MeV/u using the MINIBALL array at the REX-ISOLDE post accelerator at CERN. This is the first measurement of the reduced transition probability of this state using this method for a neutron deficient Sn isotope. The strength of the approach lies in the excellent peak-to-background ratio that is achieved. The extracted reduced transition probability, B(E2 : 0(+) -> 2(+)) 0.220 +/- 0.022e(2) b(2), strengthens the observation of the evolution of the B(E2) values of neutron deficient Sn isotopes that was observed recently in intermediate-energy Coulomb excitation of Sn-108. It implies that the trend of these reduced transition probabilities in the even-even Sn isotopes is not symmetric with respect to the midshell mass number A = 116 as Sn-100 is approached.

https://doi.org/10.1103/physrevlett.98.172501