Studies of F18 from the O16(He3,pγ)F18 Reaction

J. W. Olness and E. K. Warburton
Phys. Rev. 151, 792 – Published 18 November 1966
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Abstract

The Doppler-shift attenuation method was used to investigate the lifetimes of various gamma-ray-emitting states of F18 populated via the O16(He3,pγ)F18 reaction at a He3 bombarding energy of 3.4 MeV. Gamma-ray spectra were measured with a lithium-drifted germanium spectrometer for detection angles θγ=8 and γγ=172 relative to the incident beam direction. The results determine the mean lifetimes (in picoseconds) for the levels of F18, identified by their excitation energies (in MeV) as follows: 1.70 (0.86 ±0.20); 2.10 (4.1±1.6); 2.53 (0.67±0.18); 3.06 (<0.17); 3.35 (0.46±0.10); and 3.84 (<0.073). For each of the four longer-lived levels, the mean life was also determined from a theoretical fit to the experimental line shapes; these results have been incorporated in the values quoted for the 1.70-, 2.10-, 2.53-, and 3.35- MeV levels. The particle-gamma angular-correlation method of Litherland and Ferguson was used to gain information on the decay modes and spin assignments of the levels of F18 below an excitation energy of 3.4 MeV. Protons were detected with an annular counter at 180° to the He3 beam and gamma rays were detected at several angles between 0° and 90° to the beam. Measurements were carried out for He3 bombarding energies of 3.44, 4.65, and 5.40 MeV. These results establish spin assignments of J=2 for both the 2.10- and 3.06-MeV levels of F18, and are consistent with or confirm previously established spin-parity assignments for the remaining levels as follows: 0.937 (3+), 1.70 (1+), 2.53 (2+), 3.13 (1), and 3.35 (2 or 3). It is further established that the 2.10- and 1.08-MeV levels have the same parity. The most probable spin of the 1.08-MeV level is found to be J=0 (although J=1 or 2 are not excluded) in which case the lifetime determined for the 2.10-MeV level establishes that the 2.10 → 1.08 transition are an enhanced E2 of strength approximately 20 Weisskopf units. Additional information was obtained for the mixing ratios of various groundstate and cascade transitions in F18.

  • Received 16 June 1966

DOI:https://doi.org/10.1103/PhysRev.151.792

©1966 American Physical Society

Authors & Affiliations

J. W. Olness and E. K. Warburton

  • Brookhaven National Laboratory, Upton, New York

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Issue

Vol. 151, Iss. 3 — November 1966

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