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4 works

Work: Astrophysical S factor of 3H(α,γ) 7Li

  1. Modified two-body potential approach to the peripheral direct capture astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>a</mml:mi><mml:mo>+</mml:mo><mml:mi>A</mml:mi><mml:mo>→</mml:mo><mml:mi>B</mml:mi><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:math> reaction and asymptotic normalization coefficients

    S. B. Igamov, R. Yarmukhamedov

    ArticleNuclear physics research studiesNuclear Physics A200624 citations
    ABI

  2. Determination of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mn mathvariant="bold">3</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">He</mml:mi><mml:mo>+</mml:mo><mml:mi>α</mml:mi><mml:mo>→</mml:mo><mml:msup><mml:mrow/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>Be asymptotic normalization coefficients, the nuclear vertex constants, and their application for the extrapolation of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mn mathvariant="bold">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>He(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow><mml:mi mathvariant="bold-italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="bold">γ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mn mathvariant="bold">7</mml:mn></mml:msup></mml:math>Be astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="bold-italic">S</mml:mi></mml:math>factors to the solar energy region

    Q. I. Tursunmahatov, R. Yarmukhamedov

    ArticleNuclear physics research studiesPhysical Review C20129 citations
    ABI

  3. Astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">H</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> direct capture reactions in a potential-model approach

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

    ArticleNuclear physics research studiesPhysical review. C20185 citations
    ABI

  4. Analysis of the 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical direct capture reactions in a modified potential-model approach

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

    ArticleNuclear physics research studiesNuclear Physics A20204 citations
    ABI