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32 ta ish

Ish: 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

    Maqola199930 iqtibos
    ABI

  2. Thermonuclear Reaction Rates, II

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

    Maqola197513 iqtibos
    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

    Maqola201612 iqtibos
    ABI

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

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

    Maqola201011 iqtibos
    ABI

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

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

    Maqola199910 iqtibos
    ABI

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

    D Baye, Edouard Brainis

    Maqola200010 iqtibos
    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

    MaqolaNuclear physics research studiesBulletin of the Russian Academy of Sciences Physics20098 iqtibos
    ABI

  8. Spectroscopic factors from radiative capture reactions

    C. Rolfs

    Maqola19736 iqtibos
    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

    MaqolaNuclear physics research studiesPhysical review. C20235 iqtibos
    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

    MaqolaNuclear physics research studiesNuclear Physics A20204 iqtibos
    ABI

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

    William A. Fowler

    Maqola19844 iqtibos
    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

    MaqolaNuclear physics research studiesPhysical review. C20213 iqtibos
    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

    Maqola20193 iqtibos
    ABI

  14. Cauldrons in the cosmos: nuclear astrophysics

    Maqola19883 iqtibos
    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

    Maqola20183 iqtibos
    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

    Maqola20103 iqtibos
    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

    Maqola19982 iqtibos
    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

    Maqola19972 iqtibos
    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

    Maqola19752 iqtibos
    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

    Maqola20232 iqtibos
    ABI

  21. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  22. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  23. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  24. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  25. Sarlavhasiz

    Boshqa1 iqtibos
    ABI