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Gamow-Teller transition of the proton-rich nucleus {sup 24}Si

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3442606· OSTI ID:21362026
; ; ; ; ; ;  [1]; ; ; ; ; ;  [2]; ;  [3];  [4]; ;  [5]; ;  [6]
  1. RIKEN Nishina Center, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
  2. Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan)
  3. Variable Energy Cyclotron Centre, 1/AF, Bidhan, Nagar, Kolkata-700 064 (India)
  4. Department of Physics and Astronomy, and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321 (United States)
  5. Center for Nuclear Study, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan)
  6. Department of Physics, Tokyo Institute of Technology, 2-12-1 Oh-okayama, Meguro, Tokyo 152-8551 (Japan)
The Gamow-Teller transition strength B(GT) of {sup 24}Si was measured to investigate characteristic structure of proton-rich nuclei induced by a weakly-bound proton. By combining the results of the delayed gamma-ray and proton measurements, the entire decay scheme of {sup 24}Si was reconstructed, then the B(GT) of {sup 24}Si was deduced. Focusing to the low-lying states, the B(GT) of {sup 24}Si to the 1{sub 1}{sup +} and 1{sub 2}{sup +} states in {sup 24}Al were smaller than that of the mirror nucleus {sup 24}Ne by 22% and 10%, respectively. The mirror asymmetry of B(GT) indicates the configuration change in the wave function. Through the comparison with theoretical shell-model calculations, it is implied that the configuration change is attributed to the lowering of the 1s{sub 1/2} orbital. The applicability of the theoretical calculations was checked using overall B(GT) distribution.
OSTI ID:
21362026
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1235; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English