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NSR database version of April 29, 2024.

Search: Author = M.Serfling

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2018WA03      Phys.Rev. C 97, 015801 (2018)

L.Wagner, S.Akhmadaliev, M.Anders, D.Bemmerer, A.Caciolli, St.Gohl, M.Grieger, A.Junghans, M.Marta, F.Munnik, T.P.Reinhardt, S.Reinicke, M.Roder, K.Schmidt, R.Schwengner, M.Serfling, M.P.Takacs, T.Szucs, A.Vomiero, A.Wagner, K.Zuber

Astrophysical S factor of the ¹⁴N(p, γ)¹⁵0 reaction at 0.4-1.3 MeV

NUCLEAR REACTIONS ¹⁴N(p, γ), E=4001400 keV from tandem accelerator at Helmholtz-Zentrum Dresden-Rossendorf (HZDR); measured Eγ, Iγ, γ(θ), σ(E), resonance yields. ¹⁵O; deduced levels, proton-resonances, astrophysical S factors. R-matrix analysis. Comparison with previous experimental results.

doi: 10.1103/PhysRevC.97.015801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2439.