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NSR database version of May 1, 2024.

Search: Author = I.Hornyak

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2017GY01      Phys.Rev. C 95, 035805 (2017)

Gy.Gyurky, A.Ornelas, Zs.Fulop, Z.Halasz, G.G.Kiss, T.Szucs, R.Huszank, I.Hornyak, I.Rajta, I.Vajda

Cross section measurement of the astrophysically important ¹⁷O(p, γ)¹⁸F reaction in a wide energy range

NUCLEAR REACTIONS ¹⁷O(p, γ)¹⁸F, E=500-1800 keV; measured Eγ, Iγ, half-life of ¹⁸F decay, σ(E) by activation method using Van de Graaff accelerator of Atomki; analyzed using R-matrix fit; deduced S factors. Comparison with previous experimental data. Relevance to hydrogen burning processes in different stages of stellar evolution.

doi: 10.1103/PhysRevC.95.035805
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4367.