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Title: Gamow-Teller transitions studied in the high-resolution {sup 64}Ni({sup 3}He,t){sup 64}Cu reaction

Journal Article · · Physical Review. C, Nuclear Physics
; ; ;  [1]; ; ;  [2]; ; ;  [3];  [4]; ;  [5]; ; ; ; ; ; ;  [6]
  1. Vakgroep Subatomaire en Stralingsfysica, Universiteit Gent, B-9000 Gent (Belgium)
  2. Department of Physics, Osaka University, Toyonaka, Osaka 560-0043 (Japan)
  3. KVI, University of Groningen, NL-9747 AA Groningen (Netherlands)
  4. IKP Koeln University, Koeln (Germany)
  5. Institut fuer Kernphysik, Westfaelische Wilhelms-Universitaet Muenster, D-48149 Muenster (Germany)
  6. RCNP, Osaka University, Ibaraki, Osaka 567-0047 (Japan)

To study the Gamow-Teller (GT) transitions to the pf-shell nucleus {sup 64}Cu, the {sup 64}Ni({sup 3}He,t){sup 64}Cu experiment was performed at the Research Center for Nuclear Physics (RCNP) Ring Cyclotron, Osaka, using a {sup 3}He beam of 140 MeV/nucleon. The outgoing tritons were momentum analyzed by the Grand Raiden spectrometer at 0 deg. A high energy resolution of 32 keV (full width at half-maximum) allowed the separation of individual levels in the excitation-energy region from 0 to 3.5 MeV. In addition to the ground state (gs), known to be a J{sup {pi}}=1{sup +} GT state, many low-lying states showed L=0 nature, suggesting that they are candidates for GT states. Because the GT strength B(GT) for the gs transition is known from the {beta}-decay measurement, the strengths for the excited states could be determined using the proportionality between the B(GT) and the reaction cross section extrapolated to q=0 momentum transfer. At higher excitation energies, the level density becomes high and the so-called GT giant resonance dominates the spectrum. The lower and the upper limits of the strength contained in this energy region were estimated. Our results show that less than 55% of the strength predicted by the Ikeda sum rule is located in the excitation-energy region from 0 to 17 MeV.

OSTI ID:
21293745
Journal Information:
Physical Review. C, Nuclear Physics, Vol. 79, Issue 6; Other Information: DOI: 10.1103/PhysRevC.79.064312; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2813
Country of Publication:
United States
Language:
English