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Work: Astrophysical \(S(0)\)-factors for the \(^{3}{\mathrm {He}}(\alpha ,\gamma )^{7}{\mathrm {Be}}\), \(^{3}{\mathrm {H}}(\alpha , \gamma )^{7}{\mathrm {Li}}\), and \(^{7}{\mathrm {Be}}(p, \gamma )^{8}{\mathrm {B}}\) Direct Capture Processes in a Potential Model
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
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