References quoted in the XUNDL dataset: 18F 2H(17O,A14N):XUNDL-5

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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