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Optimal ways to produce heavy and superheavy nuclei

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Abstract

Optimal reactions to produce superheavy nuclei are discussed. The models of fusion are reviewed. The dependence of calculated evaporation residue cross sections on the predicted nuclear properties is presented. The reactions are suggested to produce nuclei with \(Z=119\) and 120, and unknown isotopes of superheavy nuclei. The evaporation residue cross sections are predicted for future experiments. The relationship between the self-consistent methods and microscopic–macroscopic approaches is considered.

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Acknowledgements

We would like to express our special gratitude to our co-authors Dr. Juhee Hong, Dr. A.N. Bezbakh, Prof. P. Jachimowicz, Prof. H. Lenske, Prof. M. Kowal, Prof. L.A. Malov, Prof. W. Scheid, and Prof. S.-G. Zhou. We are also thankful to Prof. Yu.Ts. Oganessian and Prof. S. Hofmann for the initialization of some works presented here and very fruitful discussions.

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

    G. G. Adamian & N. V. Antonenko

  2. Tomsk Polytechnic University, 634050, Tomsk, Russia

    N. V. Antonenko

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  1. G. G. Adamian
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  2. N. V. Antonenko
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Correspondence to G. G. Adamian.

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Adamian, G.G., Antonenko, N.V. Optimal ways to produce heavy and superheavy nuclei. Eur. Phys. J. A 58, 111 (2022). https://doi.org/10.1140/epja/s10050-022-00764-0

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