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Title: The {beta}-delayed {alpha} spectrum of {sup 16}N and the {sup 12}C({alpha},{gamma}){sup 16}O cross section at low energies

Journal Article · · Bulletin of the American Physical Society
OSTI ID:243779

The low-energy part of the {beta}{alpha}-decay spectrum of {sup 16}N permits the determination of the {alpha}+{sup 12}C reduced width of the E{sub x}=7.12 MeV, sub-threshold state of {sup 16}O. This state, in turn, dominates the low energy p-wave capture amplitude of the astrophysically important reaction {sup 12}C({alpha},{gamma}){sup 16}O. The {alpha}-spectrum following the decay of {sup 16}N has been measured by producing a low-energy {sup 16}N beam with the TRIUMF isotope separator TISOL, stopping the {sup 16}N nuclei in a foil, rotating it, and counting the {alpha}-particles and {sup 12}C recoil nuclei, in coincidence, in thin surface-barrier detectors. In addition to obtaining the {alpha}-spectrum, the authors determine the detector response by this method. These data, which includes 10{sup 6} {alpha}-{sup 12}C coincidences, show that the main {alpha}-peak is accompanied by a lower-energy interference structure, as predicted by several authors. The spectrum obtained has been fitted by a K-matrix parameterization which includes the measured {sup 12}C({alpha},{gamma}){sup 16}O cross sections. A value of S{sub E1}(0.3)=57{+-}13 keV{center_dot}b has been derived for the E1 part of the {sup 12}C({alpha},{gamma}){sup 16}O S factor at E{sub c.m.}0.3 MeV.

OSTI ID:
243779
Report Number(s):
CONF-9304297-; ISSN 0003-0503; TRN: 96:002199-0294
Journal Information:
Bulletin of the American Physical Society, Vol. 38, Issue 2; Conference: 1993 joint meeting of the American Physical Society and the American Association of Physics Teachers, Washington, DC (United States), 12-15 Apr 1993; Other Information: PBD: Apr 1993
Country of Publication:
United States
Language:
English