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Ish: 2H(6He,7Li)n, 12C(7Li, 6He)13N reactions and 12C(p,γ)13N astrophysical S(E) factors

1. Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor

   S. V. Artemov, R. Yarmukhamedov, N. Burtebayev +22

   MaqolaNuclear physics research studiesThe European Physical Journal A20224 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.286718

2. Astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor and reaction rate of the direct <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mn>13</mml:mn></mml:mmultiscripts></mml:math> capture process within a potential-model approach

   E. M. Tursunov, S. A. Turakulov, A. S. Kadyrov

   MaqolaNuclear physics research studiesPhysical review. C20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.006642