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6 ta ish

Ish: Activation measurement of the reaction cross section at high energies

  1. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

    G. Kiss, M. La Cognata, C. Spitaleri +38

    MaqolaNuclear physics research studiesPhysics Letters B20205 iqtibos
    ABI

  2. 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

    MaqolaNuclear physics research studiesPhysical review. C20185 iqtibos
    ABI

  3. 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

    MaqolaNuclear physics research studiesNuclear Physics A20204 iqtibos
    ABI

  4. A Modified activation method for reaction total cross section and yield measurements at low astrophysically relevant energies

    S. V. Artemov, S. B. Igamov, A. Karakhodjaev +11

    MaqolaNuclear physics research studiesNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment20161 iqtibos
    ABI

  5. Determination of the <sup>3</sup>He(<i>α</i>, <i>γ</i>)<sup>7</sup>Be and <sup>6</sup>Li(<i>p</i>, <i>γ</i>)<sup>7</sup>Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

    M. La Cognata, G. Kiss, R. Yarmukhamedov +38

    MaqolaNuclear physics research studiesEPJ Web of Conferences20230 iqtibos
    ABI

  6. Determination of the astrophysical factor of the <sup>3</sup>He(α,γ)<sup>7</sup>Be down to zero energy using the asymptotic normalization coefficient method

    M. La Cognata, G. Kiss, R. Yarmukhamedov +38

    MaqolaNuclear physics research studiesJournal of Physics Conference Series20230 iqtibos
    ABI