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40 ta ish

Ish: Influence of orthogonalization procedure on astrophysical S-factor for the direct α + d →6Li + γ capture process in a three-body model

  1. Thermonuclear Reaction Rates, II

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

    Maqola197513 iqtibos
    ABI
  2. Supersymmetry between deep and shallow nucleus-nucleus potentials

    D Baye

    Maqola198711 iqtibos
    ABI
  3. Microscopic potential model studies of light nuclear capture reactions

    K. Langanke

    Maqola19869 iqtibos
    ABI
  4. Lithium Isotopic Abundances in Metal‐poor Halo Stars

    Martin Asplund, David L. Lambert, Poul Erik Nissen +2

    Maqola20069 iqtibos
    ABI
  5. Sarlavhasiz

    Boshqa9 iqtibos
    ABI