Abstract
The neutron-rich isotopes Sc53-55 and V56-59 have been produced at GANIL in interactions of a 64.5 MeV/u Cu-65 beam with a Be-9 target. They were separated by the doubly achromatic spectrometer LISE3. Beta-decay half-lives and subsequent low-energy gamma-rays were observed for the first time. The present results are compared to QRPA model predictions. The quick drop of the half-life observed at N = 33 for Ca-53(20)33 is water V-56(23)33 and absent for Sc-54(21)33, indicating a vanishing of the N = 32 subshell north to Ca-52(32). In an astrophysical context, these neutron-rich isotopes represent r-process progenitors which, after beta-decay, would produce the correlated isotopic over-abundances of Cr-54, Fe-58, Ni-64 in certain refractory inclusions of meteorites. (C) 1998 Elsevier Science B.V.
Original language | English |
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Pages (from-to) | 205-228 |
Number of pages | 24 |
Journal | Nuclear Physics A |
Volume | 632 |
Issue number | 2 |
Publication status | Published - 16 Mar 1998 |
Keywords
- V-56,V-57.58.59(beta(-)) [from Be-9 ((CU)-C-65, X), E=64.5 MeV/nucleon] measured E gamma, I gamma,beta gamma-coin, T-1/2
- educed r-process implications
- R-PROCESS
- Sc-53.54.55
- NUCLEOSYNTHESIS
- ALLENDE METEORITE
- SPECTROMETER
- BEAM
- CA-48/CA-46 ABUNDANCE RATIO
- ANOMALIES
- STABILITY
- REGION
- ALPHA-PROCESS