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31 ta ish

Ish: Stability of superheavy nuclei produced in actinide-based complete fusion reactions: Evidence for the next magic proton number at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>⩾</mml:mo><mml:mn>120</mml:mn></mml:mrow></mml:math>

  1. Nuclear Ground-State Masses and Deformations

    P. Möller, J.R. Nix, W.D. Myers +1

    Maqola199597 iqtibos
    ABI
  2. The discovery of the heaviest elements

    S. Hofmann, G. Münzenberg

    Maqola200047 iqtibos
    ABI
  3. Heaviest nuclei from<sup>48</sup>Ca-induced reactions

    Yu. Ts. Oganessian

    Maqola200722 iqtibos
    ABI
  4. The reaction 48Ca + 238U → 286112* studied at the GSI-SHIP

    S. Hofmann, D. Ackermann, S. Antalic +24

    Maqola200712 iqtibos
    ABI
  5. Nuclear properties according to the Thomas-Fermi model

    W.D. Myers, W.J. Świa̧tecki

    Maqola199610 iqtibos
    ABI
  6. The 1993 atomic mass evaluation

    G. Audi, A.H. Wapstra

    Maqola19938 iqtibos
    ABI
  7. Chemical characterization of element 112

    R. Eichler, N. V. Aksenov, A. V. Belozerov +22

    Maqola20077 iqtibos
    ABI