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1. Comparative role of the 7Li(n, γ) reaction in Big Bang nucleosynthesis
2. Astrophysical S-factor and reaction rate for 15N(p,γ)16O within the modified potential cluster model
3. Cluster model calculations of the 11C(p,γ)12N reaction rate and comparative overview
4. Influence of Resonances on the 11B (n, γ1)12B Reaction Rate
5. Influence of resonances on the 11B(n, γ)12B reaction rate. Capture to the excited states of 12B
6. Li 6 (p,γ) Be 7 reaction rate in the light of the new data of the Laboratory for Underground Nuclear Astrophysics
7. Radiative p 11C Capture Reaction Rate
8. Rate of Radiative n 12C Decay at Temperatures from 0.01 T 9 to 10 T 9
9. Reaction Rate of p 6Li Capture
10. Reaction rate of radiative n6Li capture in the temperature range from 0.01 to 10 T9
11. Reaction rate of radiative p 12C capture in a modified potential cluster model
12. Reaction rate of radiative p12N capture
13. Reaction rate of the 7Li(p,γ)8Be radiative capture at low energies
14. 12B(n,γ)13B reaction as an alternative path to astrophysical synthesis of 13C isotope
15. The reaction rate of radiative n 8Li capture in the range from 0.01 to 10 T 9
16. Estimation of radiative capture13B(n, δ30+1)14B reaction rate in the modified potential cluster model
17. Estimation of the effect of Tsallis non-extensive statistics on the 14C(n,γ)15C reaction rate
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