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Ish: Comparison of asymptotic normalization coefficients for 10B → 9B + n and 10B → 9Be + p configurations obtained from 10B(d,t)9B and 10B(d,3He)9Be reactions

  1. Compilation of phenomenological optical-model parameters 1954–1975

    C. M. Perey, F.G. Perey

    Maqola197617 iqtibos
    ABI

  2. Spectroscopic factors for the 1p shell

    S. Cohen, D. Kurath

    Maqola196716 iqtibos
    ABI

  3. Nuclear asymptotic normalization coefficients for 14N → 13C + p configurations and astrophysical S factor for radiative proton capture

    S. V. Artemov, A. G. Bajajin, S. B. Igamov +2

    MaqolaNuclear physics research studiesPhysics of Atomic Nuclei20089 iqtibos
    ABI

  4. Elastic scattering of 52 MeV deuterons

    F. Hinterberger, G. Mairle, U. Schmidt-Rohr +2

    Maqola19685 iqtibos
    ABI

  5. Comparaison des réactions (d, 3He) ET (d, t) sur quelques noyaux N = Z

    M. J. Gaillard, R. Bouché, L. Feuvrais +5

    Maqola19684 iqtibos
    ABI

  6. Method for selecting peripheral reactions dominated by the pole mechanism: Analysis of (d,t) reactions on 1p-shell and {sup 19}F nuclei

    I.R. Gulamov, A. M. Mukhamedzhanov, G. K. Nie

    Maqola19954 iqtibos
    ABI

  7. Direct nuclear reaction theories

    N. Austern

    Kitob19703 iqtibos
    ABI

  8. Asymptotic normalization coefficients from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>,<i>d</i>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction and astrophysical factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><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" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

    A. M. Mukhamedzhanov, P. Bém, V. Burjan +9

    MaqolaNuclear physics research studiesPhysical Review C20063 iqtibos
    ABI

  9. Sarlavhasiz

    Boshqa2 iqtibos
    ABI

  10. RADII AND BINDING ENERGIES OF NUCLEI IN THE ALPHA-CLUSTER MODEL

    G. K. Nie

    MaqolaOchiq kirishNuclear physics research studiesModern Physics Letters A20072 iqtibos
    ABI

  11. RADII AND BINDING ENERGIES OF NUCLEI IN THE ALPHA-CLUSTER MODEL

    G. K. Nie

    Preprint20062 iqtibos
    ABI

  12. Sarlavhasiz

    Boshqa1 iqtibos
    ABI