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2 та иш

Иш: The¹²C(α, γ)¹⁶O Reaction Rate and the Evolution of Stars in the Mass Range 0.8 ≤ <i>M</i>/<i>M</i>_⊙ ≤ 25

1. Asymptotic normalization coefficients of resonant and bound states from the phase shifts for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mi>α</mml:mi></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>scattering

   Yu. V. Orlov, B. F. Irgaziev, Л. И. Никитина

   МақолаNuclear physics research studiesPhysical review. C20164 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.198880

2. Extracting the complex energy of broad resonances by the S-matrix pole method

   B. F. Irgaziev, A. M. Mukhamedzhanov, Yu. V. Orlov +1

   МақолаQuantum chaos and dynamical systemsBulletin of the Russian Academy of Sciences Physics20111 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.364290