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Z. Hons

8 ta ish

Nuclear Physics Institute of the Czech Academy of Sciences, 250 68 Řež, Czech Republic

  1. Indirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</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: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> reaction using the asymptotic normalization coefficient method

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

    MaqolaNuclear physics research studiesPhysical review. C20217 iqtibos
    ABI

  2. 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

  3. The full structure of the KLL Auger spectrum of La observed in the radioactive decay of 139Ce in a solid matrix

    A. Kh. Inoyatov, L.L. Perevoshchikov, A. Kovalı́k +4

    MaqolaX-ray Spectroscopy and Fluorescence AnalysisJournal of Electron Spectroscopy and Related Phenomena20133 iqtibos
    ABI

  4. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction

    R. G. Pizzone, C. Spitaleri, L. Lamia +17

    MaqolaSuperconducting Materials and ApplicationsAIP conference proceedings20100 iqtibos
    ABI

  5. First results of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>ν</mml:mi><mml:mi>GeN</mml:mi></mml:mrow></mml:math> experiment on coherent elastic neutrino-nucleus scattering

    I. Alekseev, K. Balej, V. Belov +21

    MaqolaNeutrino Physics ResearchPhysical review. D/Physical review. D.20220 iqtibos
    ABI

  6. 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

  7. 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

  8. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>π</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:math> Coulomb interaction study and its use in data processing

    B. Adeva, L. Afanasyev, A. Anania +52

    MaqolaHigh-Energy Particle Collisions ResearchPhysical review. D/Physical review. D.20240 iqtibos
    ABI