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Иш: 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

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  2. Thermonuclear Reaction Rates, II

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  10. How unique is the asymptotic normalization coefficient method?

    J.C.S. Fernandes, R. Crespo, F. M. Nunes

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    M. Agostini, B. Neumair, S. Appel +89

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  12. Polarization and phase shifts in 12C(p,p)12C and 16O(p,p)16O from 1.5 to 3 MeV

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