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NSR database version of April 27, 2024.

Search: Author = L.A.Van Wormer

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2003BL11      Nucl.Phys. A718, 127c (2003)

J.C.Blackmon, D.W.Bardayan, W.Bradfield-Smith, R.Brummitt, A.E.Champagne, A.A.Chen, T.Davinson, L.Dessieux, M.W.Guidry, K.I.Hahn, G.M.Hale, W.R.Hix, R.L.Kozub, Z.Ma, P.D.Parker, G.Rajbaidya, R.C.Runkle, C.M.Rowland, A.C.Shotter, M.S.Smith, L.A.Van Wormer, D.W.Visser, P.J.Woods

The ¹⁴O(α, p)¹⁷F Reaction Rate

NUCLEAR REACTIONS ¹H(¹⁷F, ¹⁷F), (¹⁷F, ¹⁷F'), (¹⁷F, ¹⁴O), E(cm) ≈ 1-4 MeV; measured particle spectra. ¹⁷F(p, p'), E(cm)=2-2.5 MeV; deduced σ. ¹⁴O(α, p), E=low; deduced astrophysical reaction rate. R-matrix analysis.

doi: 10.1016/S0375-9474(03)00689-4
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1138.

2002SM11      Nucl.Instrum.Methods Phys.Res. A488, 342 (2002)

D.L.Smith, D.G.Naberejnev, L.A.Van Wormer

Large Errors and Severe Conditions

RADIOACTIVITY ⁵³V(β^-); analyzed T_1/2 uncertainties.

NUCLEAR REACTIONS ³¹P(p, γ), E not given; analyzed astrophysical reaction rates, uncertainties.

doi: 10.1016/S0168-9002(02)00467-9
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