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Shell model at GAMMASPHERE: Studies in the A {approx} 96 region

Conference ·
OSTI ID:231334
; ;  [1]
  1. Notre Dame Univ., IN (United States). Dept. of Physics; and others
High-spin states in {sup 94,95}Mo, {sup 94,95,96}Tc, {sup 96,97,98}Ru and {sup 97,98}Rh were populated via the {sup 65}Cu({sup 36}S, xpyn) reactions at 142 MeV. We have observed about 300 new transitions belonging to these nuclei, and their level schemes have been extended up to a spin of J {approx} 20{h_bar} and an excitation energy of E{sub x} {approx} 12--14 MeV. Information on the high spin structure for {sup 96}Tc and {sup 98}Rh has been obtained for the first time. Spherical shell model calculations have been performed and compared with the experimental excitation energies. The level structures of the N = 51,52 isotones exhibit single-particle nature, even at high spins and excitation energies (J {approx} 20{h_bar}, E{sub x} {approx} 12--14 MeV). A fragmentation of intensity into several branches after the breaking of the N = 50 core has been observed. There are indications for the onset of collectivity around neutron number N = 53 in this mass region. A sequence of E2 transitions, indicating an onset of the vibrational degree of freedom, was observed in {sup 98}Ru at spins just above the observed N = 50 core breaking.
Research Organization:
Argonne National Lab., IL (United States). Physics Div.; Tennessee Univ., Knoxville, TN (United States). Dept. of Physics
Sponsoring Organization:
USDOE, Washington, DC (United States); National Science Foundation, Washington, DC (United States)
DOE Contract Number:
FG05-87ER40361; W-31109-ENG-38
OSTI ID:
231334
Report Number(s):
ANL/PHY/CP--89517; CONF-951274--3; ON: DE96008458; CNN: PHY94-02761; PPA/DOE-93-153
Country of Publication:
United States
Language:
English

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