References quoted in the XUNDL dataset: 18F 2H(17O,A14N):XUNDL-15

3 references found.

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2010SE13

Phys.Rev. C 82, 032801 (2010)

M.L.Sergi, C.Spitaleri, M.La Cognata, A.Coc, A.Mukhamedzhanov, S.V.Burjan, S.Cherubini, V.Crucilla, M.Gulino, F.Hammache, Z.Hons, B.Irgaziev, G.G.Kiss, V.Kroha, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, N.de Sereville, E.Somorjai, S.Tudisco, A.Tumino

New high accuracy measurement of the ¹⁷O(p, α)¹⁴N reaction rate at astrophysical temperatures

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N), E=41 MeV; measured ¹⁴N spectrum, σ(θ), momentum distribution and differential σ for resonances above the ¹⁸F proton threshold. ¹⁸F; deduced resonances and levels. Comparison of experimental momentum distribution with plane-wave impulse approximation (PWIA) and distorted-wave Born approximation (DWBA) calculations. ¹⁷O(p, α)¹⁴N; deduced reaction rates of astrophysical relevance.

doi: 10.1103/PhysRevC.82.032801

2012WA38

Chin.Phys.C 36, 1603 (2012)

M.Wang, G.Audi, A.H.Wapstra, F.G.Kondev, M.MacCormick, X.Xu, B.Pfeiffer

The AME2012 atomic mass evaluation (II). Tables, graphs and references

COMPILATION A=1-295; compiled, evaluated atomic mass data.

2015SE08

Phys.Rev. C 91, 065803 (2015)

M.L.Sergi, C.Spitaleri, M.La Cognata, L.Lamia, R.G.Pizzone, G.G.Rapisarda, X.D.Tang, B.Bucher, M.Couder, P.Davies, R.deBoer, X.Fang, L.Lamm, C.Ma, M.Notani, S.O'Brien, D.Roberson, W.Tan, M.Wiescher, B.Irgaziev, A.Mukhamedzhanov, J.Mrazek, V.Kroha

Improvement of the high-accuracy ¹⁷O(p, α)¹⁴N reaction-rate measurement via the Trojan Horse method for application to ¹⁷O nucleosynthesis

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N)n, E=41, 43.5 MeV; measured particle spectra, (¹⁴N)α-coin at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced Q-value spectra, yields as function of ¹⁴N and α emission angles, E(¹⁴N-α) versus E(α-n) plots, neutron momentum distributions, (¹⁴N)α-coincidence yields for different neutron momentum ranges, differential σ(E) of the Trojan-Horse reaction. ¹⁸F; deduced parameters for the two resonance levels, resonance strengths for the 65-keV resonance. ¹⁷O(p, α)¹⁴N; deduced reaction rates via Trojan Horse Method (THM). ¹⁸F; compiled resonance energies, J, π, Γ_p, Γ_α, Γ_γ for 24 resonances from -3.12 keV to 1684.5 keV. Relevance to destruction of ¹⁷O and the formation of ¹⁸F in stellar sites.

doi: 10.1103/PhysRevC.91.065803