Phys.Rev. C62, 055804 (2000)

D.W.Bardayan, J.C.Blackmon, C.R.Brune, A.E.Champagne, A.A.Chen, J.M.Cox, T.Davinson, V.Y.Hansper, M.A.Hofstee, B.A.Johnson, R.L.Kozub, Z.Ma, P.D.Parker, D.E.Pierce, M.T.Rabban, A.C.Shotter, M.S.Smith, K.B.Swartz, D.W.Visser, P.J.Woods

The Astrophysically Important 3⁺ State in ¹⁸Ne and the ¹⁷F(p, γ)¹⁸Ne Stellar Rate

NUCLEAR REACTIONS ¹H(¹⁷F, ¹⁷F), (¹⁷F, p), E=9-12 MeV; measured recoil proton spectra, angular distributions, (proton)(fluorine)-coin. ¹⁸Ne; deduced resonance J, π. ¹⁷F(p, γ), E not given; calculated astrophysical reaction rates. ¹H(¹⁷O, ¹⁷O), E=10.1, 12.2 MeV; measured proton angular distributions. Silicon detector array.

doi: 10.1103/PhysRevC.62.055804