References quoted in the XUNDL dataset: 18F 17O(P,G):XUNDL-20
4 references found.
Clicking on a keynumber will list datasets that reference the given article.
Nucl.Phys. A288, 317 (1977)
I.Berka, K.P.Jackson, C.Rolfs, A.M.Charlesworth, R.E.Azuma
Isospin Mixing of the 5605 and 5668 keV States in 18F in the Light of a New State at 5603 keV
NUCLEAR REACTIONS 14N(α, γ), E=1.51-1.62 MeV; measured Eγ, Iγ(θ). 17O(p, γ), E=0.56 MeV; measured Eγ, Iγ. 18F levels deduced J, π, δ, T, Γ. Natural, enriched targets.
doi: 10.1016/0375-9474(77)90138-5
Nucl.Phys. A343, 79 (1980)
H.-B.Mak, G.T.Ewan, H.C.Evans, J.D.MacArthur, W.McLatchie, R.E.Azuma
The Alpha Widths of the 5603, 5605 and 5668 keV States in 18F
NUCLEAR REACTIONS 14N(α, α), E=1.5, 1.6 MeV; measured σ(θ, Eα). 18F resonances deduced Γα. R-matrix formalism. Differentially pumped natural nitrogen gas target.
doi: 10.1016/0375-9474(80)90641-7
Phys.Rev. C 75, 035810 (2007)
A.Chafa, V.Tatischeff, P.Aguer, S.Barhoumi, A.Coc, F.Garrido, M.Hernanz, J.Jose, J.Kiener, A.Lefebvre-Schuhl, S.Ouichaoui, N.de Sereville, J.-P.Thibaud
Experimental determination of the 17O(p, α)14N and 17O(p, γ)18F reaction rates
NUCLEAR REACTIONS 14N(α, γ), E=1620-1775 keV; measured Eγ, Iγ; deduced resonance parameters. 17O(p, α), E=194-204 keV; measured Eα, σ(E, θ); deduced resonance energy, strength. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.75.035810
Phys.Rev.Lett. 133, 052701 (2024)
R.M.Gesue, G.F.Ciani, D.Piatti, A.Boeltzig, D.Rapagnani, M.Aliotta, C.Ananna, L.Barbieri, F.Barile, D.Bemmerer, A.Best, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Casaburo, F.Cavanna, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, G.M.De Gregorio, D.Dell'Aquila, 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, J.Marsh, E.Masha, R.Menegazzo, D.Mercogliano, V.Paticchio, R.Perrino, P.Prati, V.Rigato, D.Robb, L.Schiavulli, R.S.Sidhu, J.Skowronski, O.Straniero, T.Szucs, S.Zavatarelli, for the LUNA Collaboration
First Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p, γ)18F Reaction
NUCLEAR REACTIONS 17O(p, γ), E<400 KeV; measured reaction products, Eγ, Iγ; deduced σ, thick target yields, resonance parameters. Comparison with available data. The Laboratory for Underground Nuclear Astrophysics (LUNA), located at the Laboratori Nazionali del Gran Sasso (LNGS, Italy).
doi: 10.1103/PhysRevLett.133.052701