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NSR database version of April 29, 2024.

Search: Author = M.G.Kohan

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2019GY05      Phys.Rev. C 100, 015805 (2019)

Gy.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, A.Csik, Zs.Torok, R.Huszank, M.G.Kohan, L.Wagner, Zs.Fulop

Resonance strengths in the 14N(p, γ)15O astrophysical key reaction measured with activation

NUCLEAR REACTIONS 14N(p, γ)15O, E=278, 1058 keV; measured Eγ, Iγ, resonance strengths using activation method at the Institute for Nuclear Research, Debrecen. Comparison with previous experimental values. Discussion of relevance to stellar hydrogen burning.

doi: 10.1103/PhysRevC.100.015805
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4405. Data from this article have been entered in the XUNDL database. For more information, click here.


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