References quoted in the XUNDL dataset: 18O 12C(18O,18O):XUNDL-12
2 references found.
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Phys.Rev. C 89, 025809 (2014)
T.Al-Abdullah, F.Carstoiu, X.Chen, H.L.Clark, C.A.Gagliardi, Y.-W.Lui, A.Mukhamedzhanov, G.Tabacaru, Y.Tokimoto, L.Trache, R.E.Tribble, Y.Zhai
Astrophysical reaction rate for 17F(p, γ)18Ne from the transfer reaction 13C(17O, 18O)12C
NUCLEAR REACTIONS 13C(17O, 18O), 12C(18O, 18O), E=12 MeV/nucleon; measured particle spectra using multipole dipole-multipole (MDM) magnetic spectrometer, σ(θ) at Texas A and M facility. 18O; deduced levels, J, asymptotic normalization coefficients (ANCs) of ground state, first two 2+ states and first 4+ state. 17F(p, γ)18Ne, at T9=0.1-1; deduced reaction rates, astrophysical S factor from mirror analogy of states in 18O and 18Ne. Optical model parameters and DWBA analysis. Discussed production of 18F at stellar energies in ONe novae.
doi: 10.1103/PhysRevC.89.025809
Phys.Rev. C 89, 064602 (2014)
T.Al-Abdullah, F.Carstoiu, C.A.Gagliardi, G.Tabacaru, L.Trache, R.E.Tribble
Peripheral elastic and inelastic scattering of 17, 18O on light targets at 12 MeV/nucleon
NUCLEAR REACTIONS 13C(17O, 18O), E=12 MeV/nucleon; 12C(18O, 18O), (18O, 18O'), E=216 MeV; 13C(17O, 17O), (17O, 17O'), E=204 MeV; measured particle spectra, σ, σ(θ). 12C(16O, 16O), E=18 MeV/nucleon; analyzed previous σ(θ) data; deduced form factors, optical model parameters, WKB scattering amplitude, semiclassical absorption profile for WS potential, Argand diagram for S-matrix. Analysis by semimicroscopic double folding form factors, using six different approximations for the NN effective interactions. DWBA analysis of σ(θ) data. 17,18O; deduced levels, J, π, deformation parameters. Relevance of 13C(17O, 18O) transfer reaction in deducing direct capture rates in 17F(p, γ)18Ne reaction of astrophysical importance, and influence on abundances of 15O, 17F, 18F and 18Ne.
doi: 10.1103/PhysRevC.89.064602