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Работ: 15

Работа: 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

    СтатьяNuclear physics research studiesPhysical Review C2012Цитирований: 9
    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

    СтатьяNuclear physics research studiesPhysical review. C2016Цитирований: 8
    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

    СтатьяNuclear physics research studiesPhysics Letters B2020Цитирований: 5
    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

    СтатьяNuclear physics research studiesPhysical review. C2018Цитирований: 5
    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

    СтатьяNuclear physics research studiesNuclear Physics A2020Цитирований: 4
    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

    СтатьяNuclear physics research studiesPhysical review. C2021Цитирований: 3
    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

    СтатьяNuclear physics research studiesPhysics of Atomic Nuclei2018Цитирований: 3
    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

    СтатьяNuclear physics research studiesNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment2016Цитирований: 1
    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

    СтатьяNuclear physics research studiesModern Physics Letters A2026Цитирований: 1
    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

    СтатьяNuclear physics research studiesInternational Journal of Modern Physics Conference Series2019Цитирований: 1
    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

    СтатьяNuclear physics research studiesActa Physica Polonica B2013Цитирований: 0
    ABI

  12. Indirect Methods and ANCs for Nuclear Astrophysics

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

    СтатьяNuclear physics research studiesProceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)2017Цитирований: 0
    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

    СтатьяNuclear physics research studiesEPJ Web of Conferences2023Цитирований: 0
    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

    СтатьяNuclear physics research studiesJournal of Physics Conference Series2023Цитирований: 0
    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

    СтатьяNuclear physics research studiesPhysical review. C2025Цитирований: 0
    ABI