First beta-decay studies of the neutron-rich isotopes Sc53-55 and V56-59

O. Sorlin, V. Borrel, S. Grevy, D. Guillemaud-Mueller, A.C. Mueller, F. Pougheon, W. Bohmer, K.L. Kratz, T. Mehren, P. Moller, B. Pfeiffer, T. Rauscher, M.G. Saint-Laurent, R. Anne, M. Lewitowicz, A. Ostrowski, T. Dorfler, W.D. Schmidt-Ott

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44 Citations (Scopus)

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 languageEnglish
Pages (from-to)205-228
Number of pages24
JournalNuclear Physics A
Volume632
Issue number2
Publication statusPublished - 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

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