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

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

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

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Background: The N-14(p, gamma)O-15 reaction plays a vital role in various astrophysical scenarios. Its reaction rate must be accurately known in the present era of high precision astrophysics. The cross section of the reaction is often measured relative to a low energy resonance, the strength of which must therefore be determined precisely.

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《Physical review, C》 |2019年第1期|共8页
作者
Gyurky Gy; Halasz Z.; Kiss G. G.Szucs T.Csik A.Torok ZsHuszank R.Kohan M. G.Wagner L.Fulop Zs;
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作者单位

Inst Nucl Res Atomki, H-4001 Debrecen, Hungary;

Lulea Univ Technol, Dept Engn Sci & Math, S-97187 Lulea, Sweden;

HZDR, D-01328 Dresden, Germany;

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正文语种英语
中图分类原子核物理学、高能物理学;
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1. Astrophysical S-factor of N-14(p, gamma)O-15 [J] . Formicola A, Imbriani G, Costantini HAngulo CBemmerer DBonetti RBroggini CCorvisiero PCruz JDescouvemont P Physics Letters, B. Nuclear Physics and High Energy Physics . 2004,第2期

机译：Astrophysical S-factor of N-14(p, gamma)O-15
2. The N-14(p, gamma)O-15 reaction, solar neutrinos and the age of the globular clusters [J] . DeglInnocenti S, Fiorentini G, Ricci BVillante FL Physics Letters, B. Nuclear Physics and High Energy Physics . 2004,第2期

机译：The N-14(p, gamma)O-15 reaction, solar neutrinos and the age of the globular clusters
3. Astrophysical S factor of the N-14(p,gamma)O-15 reaction at 0.4-1.3 MeV [J] . Wagner L., Akhmadaliev S., Anders M., Physical review, C . 2018,第1期

机译：N-14（P，GAMMA）O-15反应的天体物理S因子在0.4-1.3 meV下反应
4. Publisher's Note: Asymptotic normalization coefficients for N-14+p -> O-15 and the astrophysical S factor for N-14(p,gamma)O-15 (vol 67, art no 065804, 2003) [O] . Mukhamedzhanov, AM, Bem, P., Brown, BA, 2003

机译：发行者的注释：N-14 + p-> O-15的渐近归一化系数和N-14（p，gamma）O-15的天体S因子（第67卷，艺术品编号0680804，2003）

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

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