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Иш: Study of the direct 16O(p,γ)17F astrophysical capture reaction within a potential model approach

  1. A compilation of charged-particle induced thermonuclear reaction rates

    C. Angulo, M. Arnould, M. Rayet +25

    Мақола199930 иқтибос
    ABI

  2. Thermonuclear Reaction Rates, II

    William A. Fowler, Georgeanne R. Caughlan, Barbara A. Zimmerman

    Мақола197513 иқтибос
    ABI

  3. Primordial<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>γ</mml:mi></mml:mrow></mml:math>reaction and second lithium puzzle

    A. M. Mukhamedzhanov, R. Chatterjee Shubhchintak, C. A. Bertulani

    Мақола201612 иқтибос
    ABI

  4. Radiative capture of nucleons at astrophysical energies with single-particle states

    Jin Tao Huang, C. A. Bertulani, V. Guimarães

    Мақола201011 иқтибос
    ABI

  5. Tests of transfer reaction determinations of astrophysical<b><i>S</i></b>factors

    C. A. Gagliardi, R. E. Tribble, A. Azhari +10

    Мақола199910 иқтибос
    ABI

  6. Zero-energy determination of the astrophysical<b><i>S</i></b>factor and effective-range expansions

    D Baye, Edouard Brainis

    Мақола200010 иқтибос
    ABI

  7. Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies

    S. V. Artemov, S. B. Igamov, K. I. Tursunmakhatov +1

    МақолаNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20098 иқтибос
    ABI

  8. Spectroscopic factors from radiative capture reactions

    C. Rolfs

    Мақола19736 иқтибос
    ABI

  9. Detailed study of the astrophysical direct capture reaction <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</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>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> in a potential model approach

    E. M. Tursunov, S. A. Turakulov, K. I. Tursunmakhatov

    МақолаNuclear physics research studiesPhysical review. C20235 иқтибос
    ABI

  10. 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

    МақолаNuclear physics research studiesNuclear Physics A20204 иқтибос
    ABI

  11. Experimental and theoretical nuclear astrophysics: the quest for the origin of the elements

    William A. Fowler

    Мақола19844 иқтибос
    ABI

  12. 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

    МақолаNuclear physics research studiesPhysical review. C20213 иқтибос
    ABI

  13. Theoretical calculation of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>p</mml:mi><mml:mo>−</mml:mo><mml:msup><mml:mrow/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:msup><mml:mrow><mml:mi mathvariant="normal">Li</mml:mi></mml:mrow></mml:math> radiative capture reaction

    Alex Gnech, L. E. Marcucci

    Мақола20193 иқтибос
    ABI

  14. Cauldrons in the cosmos: nuclear astrophysics

    Мақола19883 иқтибос
    ABI

  15. Extrapolation of scattering data to the negative-energy region. III. Application to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>−</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> system

    L. D. Blokhintsev, A. S. Kadyrov, A. M. Mukhamedzhanov +1

    Мақола20183 иқтибос
    ABI

  16. AZURE: An<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>R</mml:mi></mml:mrow></mml:math>-matrix code for nuclear astrophysics

    R.E. Azuma, E. Uberseder, E. C. Simpson +8

    Мақола20103 иқтибос
    ABI

  17. Microscopic analysis of extranuclear capture on the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>16</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">O</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>17</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">F</mml:mi></mml:math>reaction

    D Baye, P. Descouvemont, M. Hesse

    Мақола19982 иқтибос
    ABI

  18. Halo Properties of the First<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>1</mml:mn><mml:mi>/</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math>State in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>17</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>O</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>16</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="italic">p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>F</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>17</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>Reaction

    R. Morlock, R. Kunz, A. Mayer +7

    Мақола19972 иқтибос
    ABI

  19. The <sup>16</sup>O(p, γ)<sup>17</sup>F Direct Capture Cross Section with an Extrapolation to Astrophysical Energies

    H. C. Chow, G. M. Griffiths, T. H. Hall

    Мақола19752 иқтибос
    ABI

  20. Astrophysical \(S(0)\)-factors for the \(^{3}{\mathrm {He}}(\alpha ,\gamma )^{7}{\mathrm {Be}}\), \(^{3}{\mathrm {H}}(\alpha , \gamma )^{7}{\mathrm {Li}}\), and \(^{7}{\mathrm {Be}}(p, \gamma )^{8}{\mathrm {B}}\) Direct Capture Processes in a Potential Model

    S.A. Turakulov, E.M. Tursunov

    Мақола20232 иқтибос
    ABI

  21. Сарлавҳасиз

    Бошқа1 иқтибос
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  22. Сарлавҳасиз

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  23. Сарлавҳасиз

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  24. Сарлавҳасиз

    Бошқа1 иқтибос
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  25. Сарлавҳасиз

    Бошқа1 иқтибос
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