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Feature of production of new superheavy nuclei in actinide-based complete-fusion reactions

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Abstract

Within the dinuclear system model we analyse the production of unknown superheavy nuclei in various actinide-based complete-fusion reactions. Different predictions of the properties of the heaviest nuclei are used. The dependence of the calculated evaporation residue cross-sections on the predicted shell structure and magic numbers of the heaviest nuclei is discussed.

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Authors and Affiliations

  1. Joint Institute for Nuclear Research, 141980, Dubna, Russia

    G. G. Adamian & N. V. Antonenko

  2. Institute of Nuclear Physics, 702132, Tashkent, Uzbekistan

    G. G. Adamian

  3. Institut für Theoretische Physik der Justus-Liebig-Universität, D-35392, Giessen, Germany

    W. Scheid

Authors
  1. G. G. Adamian
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  2. N. V. Antonenko
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  3. W. Scheid
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Corresponding author

Correspondence to G. G. Adamian.

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T. Bíró

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Adamian, G.G., Antonenko, N.V. & Scheid, W. Feature of production of new superheavy nuclei in actinide-based complete-fusion reactions. Eur. Phys. J. A 41, 235–241 (2009). https://doi.org/10.1140/epja/i2009-10795-4

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  • DOI: https://doi.org/10.1140/epja/i2009-10795-4

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