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NSR database version of April 29, 2024.

Search: Author = H.Babu

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2023SK02      Phys.Rev. C 107, L062801 (2023)

J.Skowronski, E.Masha, D.Piatti, M.Aliotta, H.Babu, D.Bemmerer, A.Boeltzig, R.Depalo, A.Caciolli, F.Cavanna, L.Csedreki, Z.Fulop, G.Imbriani, D.Rapagnani, S.Rummler, K.Schmidt, R.S.Sidhu, T.Szucs, S.Turkat, A.Yadav

Improved S factor of the ¹²C(p, γ)¹³N reaction at E=320-620 keV and the 422 keV resonance

NUCLEAR REACTIONS ¹²C(p, γ)¹³N, E=350-670 keV; measured Eγ, Iγ, γ(θ); deduced resonance energy, resonance γ- and p-width, S-factor, astrophysical reaction rate (T=0.01-10 GK). R-matrix analysis. Relevance to HCNO nucleosynthesis.Comparison to other experimental data. Gammas detected by HPGe cluster detector. Molecular H₂⁺ beam from 5MV Pelletron accelerator of Felsenkeller Laboratory

doi: 10.1103/PhysRevC.107.L062801
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