Phys.Rev. C57, 2731 (1998); Erratum Phys.Rev. C58, 1354 (1998)

S.Utku, J.G.Ross, N.P.T.Bateman, D.W.Bardayan, A.A.Chen, J.Gorres, A.J.Howard, C.Iliadis, P.D.Parker, M.S.Smith, R.B.Vogelaar, M.Wiescher, K.Yildiz

Breakout from the Hot CNO Cycle: The ¹⁸F(p, γ) vs ¹⁸F(p, α) branching ratio

NUCLEAR REACTIONS ¹⁹F(³He, t), (³He, tα), (³He, pt), E=29.8 MeV; ¹⁶O(⁶Li, t), (⁶Li, ³He), E=32 MeV; measured particle spectra, tp-, tα-coin; deduced reaction rates for ¹⁸F + p. ¹⁹F deduced levels, resonance features. Astrophysical implications.

doi: 10.1103/PhysRevC.57.2731