6533b833fe1ef96bd129b638
RESEARCH PRODUCT
First prompt in-beam γ-ray spectroscopy of a superheavy element: the256Rf
Pauli PeuraPaul GreenleesR.-d. HerzbergJuha UusitaloF. P. HeßbergerPhilippos PapadakisCh. TheisenS. RintaAndrej HerzanM. VenhartDaniel CoxJ. PiotT. GrahnSteffen KetelhutJan SarénJ. RubertB. GallG. HenningMatti LeinoT. L. KhooR. L. LozevaB. SulignanoA. Lopez-martensR. JulinUlrika JakobssonPaivi NieminenK. HauschildJuha SorriP. RahkilaO. DorvauxC. ScholeyF. DecheryJ. LjungvallPanu RuotsalainenM. AsaiJanne PakarinenD. SeweryniakS. JuutinenMikael SandzeliusE. ParrPeter M. JonesL.-l. AnderssonZouhair Asfarisubject
PhysicsHistoryInstrumentationShell (structure)Moment of inertiaComputer Science ApplicationsEducationNuclear physicsmedicine.anatomical_structuremedicineAtomic physicsSpin (physics)SpectroscopyNucleusBeam (structure)description
Using state-of-the-art γ-ray spectroscopic techniques, the first rotational band of a superheavy element, extending up to a spin of 20 , was discovered in the nucleus 256Rf. To perform such an experiment at the limits of the present instrumentation, several developments were needed. The most important of these developments was of an intense isotopically enriched 50Ti beam using the MIVOC method. The experimental set-up and subsequent analysis allowed the 256Rf ground-state band to be revealed. The rotational properties of the band are discussed and compared with neighboring transfermium nuclei through the study of their moments of inertia. These data suggest that there is no evidence of a significant deformed shell gap at Z = 104.
year | journal | country | edition | language |
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2013-03-25 | Journal of Physics: Conference Series |