Phys. Rev. C 27, 1387 - 1393 (1983)

Gamow-Teller strength in the 18O(pn)18F reaction at 135 MeV

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B. D. Anderson, A. Fazely, R. J. McCarthy, P. C. Tandy, J. W. Watson, and R. Madey
Department of Physics, Kent State University, Kent, Ohio 44242

W. Bertozzi, T. N. Buti, J. M. Finn, J. Kelly, M. A. Kovash, and B. Pugh
Department of Physics and Laboratory for Nuclear Science Massachusetts Institute of Technology, Cambridge, Massachusetts 02139

B. H. Wildenthal
Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824

C. C. Foster
Indiana University Cyclotron Facility, Bloomington, Indiana 47405

Received 26 October 1982

The distribution of Gamow-Teller strength in the 18O(pn)18F reaction was studied at a bombarding energy of 135 MeV. Five 1+, T=0 states are identified below Ex=7 MeV and a concentration of 1+ states of presumed T=1 character is observed between Ex=9.5 and 12 MeV. Approximately 82% of the 1+ strength is concentrated into the ground-state transition and only 5.5% is seen in the T=1 component. Normalization of the ground-state transition to the known Gamow-Teller matrix element from the analogous beta decay of 18Ne allows the (pn) cross sections to be related to the Gamow-Teller strength. The resulting total Gamow-Teller strength observed in the (pn) reaction is about two-thirds of the minimum value required by the sum rule for a T=1 nucleus. This result is in reasonable agreement with the total Gamow-Teller strength predicted from a shell-model calculation which uses empirically renormalized single-particle Gamow-Teller matrix elements. The concentration of the T=0 strength predominantly into the ground state and the observed ratio of T=1 to T=0 strength also are consistent with these calculations.

NUCLEAR REACTIONS 18O(pn)18F, E=135 MeV; neutron spectra measured in ∼3° steps between 0° and 69°; angular distributions extracted for separate transitions. Strengths of forward-peaked transitions compared with shell-model predictions of Gamow-Teller strength.


©1983 The American Physical Society

URL: http://link.aps.org/abstract/PRC/v27/p1387
DOI: 10.1103/PhysRevC.27.1387

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