References quoted in the XUNDL dataset: 18F 17O(P,G),(P,A):RES:XUNDL-22
7 references found.
Clicking on a keynumber will list datasets that reference the given article.
Nucl.Phys. A217, 29 (1973)
C.Rolfs
Spectroscopic Factors from Radiative Capture Reactions
NUCLEAR REACTIONS 16O(p, γ), E=0.3-3.1 MeV; measured σ(E), Eγ, Iγ, Iγ(θ). 17O(p, γ), E=0.3-1.9 MeV; measured σ(E), Eγ, Iγ, Iγ(θ). 17F, 18F levels deduced L, J, γ-branching, S. Natural, depleted, enriched targets.
doi: 10.1016/0375-9474(73)90622-2
Nucl.Phys. A331, 155 (1979)
W.E.Kieser, R.E.Azuma, K.P.Jackson
The 17O(p, α)14N Reaction: Physics and Astrophysics
NUCLEAR REACTIONS 17O(p, α), E=0.4-1.4 MeV; measured Iα, absolute γ-transition strength. 18F resonances deduced E, Γp, Γα.
doi: 10.1016/0375-9474(79)90307-5
Phys.Rev. C 81, 045801 (2010)
J.R.Newton, C.Iliadis, A.E.Champagne, J.M.Cesaratto, S.Daigle, R.Longland
Measurement of 17O(p, γ)18F between the narrow resonances at Erlab=193 and 519 keV
NUCLEAR REACTIONS 17O(p, γ)18O, E=151, 275, 300, 325, 400, 450, 500, 519 keV; measured Eγ, Iγ; deduced levels, total yields, σ, and total S factors. Compared with previous work.
doi: 10.1103/PhysRevC.81.045801
Phys.Rev. C 85, 035803 (2012)
U.Hager, L.Buchmann, B.Davids, J.Fallis, B.R.Fulton, N.Galinski, U.Greife, D.A.Hutcheon, D.Ottewell, A.Rojas, C.Ruiz, K.Setoodehnia
Measurement of the 17O(p, γ)18F reaction rate at astrophysically relevant energies
NUCLEAR REACTIONS 1H(17O, γ)18F, E(cm)=250-500 keV; measured 18F spectra, time-of-flight, energy loss, Eγ, Iγ, (18F)γ-coin; deduced levels, branching ratios to capture states, charge-state distributions, astrophysical S factors. DRAGON facility at TRIUMF. GEANT3 simulations for γ-ray events in BGO array. Comparison with earlier measurements.
doi: 10.1103/PhysRevC.85.035803
Phys.Rev. C 91, 015812 (2015)
M.Q.Buckner, C.Iliadis, K.J.Kelly, L.N.Downen, A.E.Champagne, J.M.Cesaratto, C.Howard, R.Longland
High-intensity-beam study of 17O(p, γ)18F and thermonuclear reaction rates for 17O + p
NUCLEAR REACTIONS 17O(p, γ), E=170-530 keV; measured Eγ, Iγ, γγ-coin at LENA-TUNL facility. 18F; deduced levels, J, π, resonances, γ branching ratios from resonance capture, and from direct capture as function of E(p), resonance strengths, total S(E) factors. 17O(p, γ), (p, α); deduced thermonuclear reaction rates. Comparison with previous results.
doi: 10.1103/PhysRevC.91.015812
Phys.Rev. C 95, 035805 (2017)
Gy.Gyurky, A.Ornelas, Zs.Fulop, Z.Halasz, G.G.Kiss, T.Szucs, R.Huszank, I.Hornyak, I.Rajta, I.Vajda
Cross section measurement of the astrophysically important 17O(p, γ)18F reaction in a wide energy range
NUCLEAR REACTIONS 17O(p, γ)18F, E=500-1800 keV; measured Eγ, Iγ, half-life of 18F decay, σ(E) by activation method using Van de Graaff accelerator of Atomki; analyzed using R-matrix fit; deduced S factors. Comparison with previous experimental data. Relevance to hydrogen burning processes in different stages of stellar evolution.
doi: 10.1103/PhysRevC.95.035805
Phys.Rev. C 111, 025805 (2025)
D.Rapagnani, O.Straniero, G.Imbriani, M.Aliotta, C.Ananna, F.Barile, L.Barbieri, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Casaburo, F.Cavanna, G.F.Ciani, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, R.M.Gesue, Gy.Gyurky, A.Guglielmetti, C.Gustavino, M.Junker, M.Lugaro, P.Marigo, J.Marsh, E.Masha, R.Menegazzo, D.Mercogliano, V.Paticchio, D.Piatti, P.Prati, V.Rigato, D.Robb, R.S.Sidhu, J.Skowronski, T.Szucs, S.Zavatarelli, for the LUNA Collaboration
Revision of the CNO cycle: Rate of 17O destruction in stars
doi: 10.1103/PhysRevC.111.025805