Abstract No: |
001
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Submitted on: |
2 Nov 2000, 9:15 GMT
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Title: |
The structure of high-Z nuclei from studies with GAMMASPHERE at ATLAS
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Author(s): |
Robert V. F. Janssens
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Affiliation(s): |
Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA
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This presentation will review one of the main research programs carried
out with the Gammasphere array at ATLAS. Taking advantage of the
availability of very heavy beams on the one hand, and of the coupling
of Gammasphere with the Fragment Mass Analyzer on the other, it was
possible to gain new insights into the properties of
actinide and transfermium nuclei.
Coulomb excitation measurements with 207,208Pb beams at energies 15 above the barrier have been carried out on 232Th and on long-lived Pu targets with A = 239, 240, 242, and 244. In addition to the target excitations, transfer channels leading to 238,241,243Pu were studied as well. With a 209Bi beam, the level structures of 237Np, 241Am and of the one-proton transfer channel leading to 242Cm were investigated. Several surprising results concerning the behavior of the negative parity bands and of band structures built on the first excited 0+ states will be discussed.
The recoil decay tagging technique was used to study not only the yrast structure of Z=102 isotopes 253No and 254No, but also the entry distributions using 48Ca + 207,208Pb fusion-evaporation reactions. The results confirm that the shell-correction energy responsible for the stability of No is partly derived from deformation. Based on a novel approach to determine a lower bound of the barrier height, the measured entry distributions provide direct information on the reaction mechanism(s), the fission barrier and the shell-correction energy. The results will be compared with theoretical expectations.
Finally, several single-particle and vibrational states above the N=152 subshell gap were investigated by combining the results from - spectroscopy following the decay of 255Fm to 251Cf with cross section data for the 250Cf(d,p) reaction.
This work is supported by the U.S. Department of Energy, Nuclear Physics Division, under Contracts No. W-31-109-ENG-38.