References quoted in the XUNDL dataset: 19F 18O(P,A):XUNDL-17
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Z.Phys. A351, 453 (1995)
H.W.Becker, M.Bahr, M.Berheide, L.Borucki, M.Buschmann, C.Rolfs, G.Roters, S.Schmidt, W.H.Schulte, G.E.Mitchell, J.S.Schweitzer
Hydrogen Depth Profiling using 18O Ions
NUCLEAR REACTIONS, ICPND 1H(15N, α), E=6.58 MeV; 1H(18O, α), E=2.9 MeV; measured spectra. 18O(p, α), E ≈ 140-160 keV; calculated astrophysical S-factor vs E. 1H(15N, α), E ≈ 6.525-6.625 MeV; 1H(18O, α), E ≈ 2.85-2.95 MeV; measured yield ratio Iα/I(H) vs E. 16O, 19F deduced more accurate resonance parameters. 1H(18O, α), E ≈ 2.68-2.78 MeV; measured α-yield vs E. 1H(15N, α), E ≈ 6.36-6.48 MeV; measured γ yield vs E. Single stage accelerator technique, depth profiling applications.
Chin.Phys.C 41, 030003 (2017)
M.Wang, G.Audi, F.G.Kondev, W.J.Huang, S.Naimi, X.Xu
The AME2016 atomic mass evaluation (II). Tables, graphs and references
ATOMIC MASSES A=1-295; compiled, evaluated atomic masses data.
doi: 10.1088/1674-1137/41/3/030003
Phys.Lett. B 790, 237 (2019)
C.G.Bruno, M.Aliotta, P.Descouvemont, A.Best, T.Davinson, D.Bemmerer, A.Boeltzig, C.Broggini, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.R.Pantaleo, D.Piatti, P.Prati, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi
Improved astrophysical rate for the 18O(p, α)15N reaction by underground measurements
NUCLEAR REACTIONS 18O(p, α)15N, E=60-360 keV; measured reaction products, Ep, Ip, Eα, Iα; deduced differential yield, resonance energies, S-factor, J, π, reaction rates.
doi: 10.1016/j.physletb.2019.01.017