PREPRINT
DB25DF34-F683-43D0-A188-0D2DBADA8723

The 15N(\bmα,\bmγ)19F reaction and nucleosynthesis of 19F

S. Wilmes, V. Wilmes, G. Staudt, P. Mohr, J. W. Hammer
arXiv:nucl-ex/0211031

Submitted on 27 November 2002

Abstract

Several resonances in the 15N(α,γ)19F reaction have been investigated in the energy range between 0.6 MeV and 2.7 MeV. Resonance strengths and branching ratios have been determined. High sensitivity could be obtained by the combination of the {\sc{dynamitron}} high current accelerator, the windowless gas target system {\sc{rhinoceros}}, and actively shielded germanium detectors. Two levels of 19F could be observed for the first time in the (α,γ) channel, and several weak branchings below the detection limits of previous experiments were measured. Two observed resonances correspond to α-cluster states in 19F which have been assigned unambiguously. The astrophysical reaction rate is derived from this set of resonance strengths.

Preprint

Comment: 9 pages, 5 figures, revtex & bibtex; Phys. Rev. C, accepted

Subjects: Nuclear Experiment; Astrophysics

URL: https://arxiv.org/abs/nucl-ex/0211031