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15 ta ish

Ish: Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles

  1. 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

    MaqolaNuclear physics research studiesPhysical Review C20129 iqtibos
    ABI

  2. Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mspace width="0.16em"/><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> from the peripheral <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and their astrophysical application

    O. R. Tojiboev, R. Yarmukhamedov, S. V. Artemov +1

    MaqolaNuclear physics research studiesPhysical review. C20168 iqtibos
    ABI

  3. 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

  4. 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

  5. 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

  6. Astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor and rate of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> direct capture reaction in a potential model

    E. M. Tursunov, S. A. Turakulov, A. S. Kadyrov +1

    MaqolaNuclear physics research studiesPhysical review. C20213 iqtibos
    ABI

  7. Asymptotic Normalization Coefficients (Nuclear Vertex Constants), Three-Body Asymptotic Normalization Functions (On-Shell Vertex Functions) and Nuclear Astrophysics

    R. Yarmukhamedov, L. D. Blokhintsev

    MaqolaNuclear physics research studiesPhysics of Atomic Nuclei20183 iqtibos
    ABI

  8. 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

  9. Asymptotic normalization coefficient for <sup>8</sup> Be→ <sup>7</sup> Li+p from the <sup>7</sup> Li( <sup>3</sup> He,d) <sup>8</sup> Be reaction and astrophysical S factor for the radiative capture <sup>7</sup> Li(p,γ) <sup>8</sup> Be reaction

    K.I. Tursunmakhatov, S.B. Igamov

    MaqolaNuclear physics research studiesModern Physics Letters A20261 iqtibos
    ABI

  10. 3He(α,γ)7Be and 3H(α,γ)7Li reaction rates and implication for Big Bang nucleosynthesis in the potential model

    S. A. Turakulov, E. M. Tursunov

    MaqolaNuclear physics research studiesInternational Journal of Modern Physics Conference Series20191 iqtibos
    ABI

  11. Odd-parity &lt;sup&gt;&lt;span class="cmr-7"&gt;100&lt;/span&gt;&lt;/sup&gt;Sn Core Excitations

    M. Palacz, J. Nyberg, H. Grawe +20

    MaqolaNuclear physics research studiesActa Physica Polonica B20130 iqtibos
    ABI

  12. Indirect Methods and ANCs for Nuclear Astrophysics

    R. Yarmukhamedov, O. R. Tojiboev, S. V. Artemov

    MaqolaNuclear physics research studiesProceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)20170 iqtibos
    ABI

  13. 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

  14. 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

  15. 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

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

    MaqolaNuclear physics research studiesPhysical review. C20250 iqtibos
    ABI