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NSR database version of May 24, 2024.

Search: Author = L.A.Van Wormer

Found 2 matches.

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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
Citations: PlumX Metrics

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 T1/2 uncertainties.

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

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


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