Phys.Rev. C 96, 025810 (2017)

S.M.Cha, K.Y.Chae, S.Ahn, D.W.Bardayan, K.A.Chipps, J.A.Cizewski, M.E.Howard, R.L.Kozub, K.Kwak, B.Manning, M.Matos, P.D.O'Malley, S.D.Pain, W.A.Peters, S.T.Pittman, A.Ratkiewicz, M.S.Smith, S.Strauss

Spectroscopic study of the radionuclide ²¹Na for the astrophysical ¹⁷F (α, p) ²⁰Ne reaction rate

NUCLEAR REACTIONS ²⁴Mg(p, α)²¹Na, E=31 MeV; measured particle spectra, Eα, Iα, σ(θ) using annular silicon strip detector array at the ORNL Holifield Radioactive Ion Beam Facility. ²¹Na; deduced levels, proton resonances, J, π, L-transfers by DWBA analysis, Γ_α and resonance strengths of proton resonances. Comparison with previous experimental data as in the Nuclear Data Sheets. ¹⁷F(α, p)²⁰Ne, T=0.1-1.1 GK; deduced astrophysical reaction rates, and compared with previous values, and with REACLIB compilation.

doi: 10.1103/PhysRevC.96.025810