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Phys. Rev. C 75, 024305 (2007) [8 pages]

Structure of 23F via β decay of 23O

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C. S. Sumithrarachchi1,2,*, D. J. Morrissey1,2, B. A. Brown1,3, A. D. Davies1,3, D. A. Davies1,2, M. Fancina1, E. Kwan1,3, P. F. Mantica1,2, M. Portillo1, Y. Shimbara1, J. Stoker1,2, and R. R. Weerasiri1,2
1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
2Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA
3Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA

Received 28 September 2006; published 15 February 2007

The nuclear states in 23F have been investigated following the β decay of 23O. The measurement of 23O was carried out at the National Superconducting Cyclotron Laboratory using fragments from the reaction of a 48Ca beam in a Be target. The half-life and total neutron emission probability were determined to be 97(8) ms and 7(2)%, respectively, for 23O β decay. Ten γ-ray decays in 23F and a single γ-ray in 22F were observed to establish the β decay scheme for 23O. Shell model calculations are in reasonable agreement with the measured β branching and B(GT) values for the lowest energy state. The excitation energies of the first 1/2+ and 3/2+ states have been determined to be 2243(8) and 4066(16) keV, respectively, indicating a widening of the 5/2+1/2+ state gap in 23F. The decay scheme of the largest contaminant 26Ne in the experiment was established.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.75.024305
DOI:
10.1103/PhysRevC.75.024305
PACS:
23.40.-s, 21.60.Cs, 23.20.Lv, 27.30.+t

*Electronic address: chandana@nscl.msu.edu