References quoted in the XUNDL dataset: 21NA 20NE(P,G):XUNDL-16
2 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev. C 97, 065802 (2018)
S.Lyons, J.Gorres, R.J.deBoer, E.Stech, Y.Chen, G.Gilardy, Q.Liu, A.M.Long, M.Moran, D.Robertson, C.Seymour, B.Vande Kolk, M.Wiescher, A.Best
Determination of 20Ne(p, γ)21Na cross sections from Ep = 500 2000 keV
NUCLEAR REACTIONS 20,22Ne(p, γ), E=500-2000 keV; measured Eγ, Iγ, γ(θ), differential σ(θ, E) at the KN accelerator of Notre Dame Nuclear Science Laboratory. 21Na; deduced levels, resonances, asymptotic normalization constants (ANCs), proton widths, γ-widths, astrophysical S-factor, and reaction rates in the range of 0.010-10.0 GK. AZURE2 R-matrix analysis. Comparison with previous experimental results, NACRE evaluation, and with theoretical predictions. Relevance to nucleosynthesis of Ne, Na, and Mg isotopes, and hydrogen burning in red giants, asymptotic giant branch (AGB) stars, massive stars, and oxygen-neon (ONe) nova.
doi: 10.1103/PhysRevC.97.065802
Phys.Rev. C 108, L052801 (2023)
E.Masha, for the LUNA collaboration
First measurement of the low-energy direct capture in 20Ne(p, γ)21Na and improved energy and strength of the Ec.m = 368 keV resonance
NUCLEAR REACTIONS 20Ne(p, γ)21Na, E(cm)=366-380 keV; measured Eγ, Iγ, γ(θ); deduced astrophysical S-factor, resonance at 368-keV c.m. energy, branching ratio from the resonance, resonance strength, thermonuclear reaction rate (T=0.5-10 GK), branching ratios. Relevance to oxygen-neon (ONe) novae simulations. Windowless neon gas target with two HPGe detectors at LUNA 400-kV accelerator (Laboratory for Underground Nuclear Astrophysics, Gran Sasso National Laboratories).
doi: 10.1103/PhysRevC.108.L052801