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Hot and cold fusion reactions leading to the same superheavy evaporation residue

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Abstract

Excitation functions are predicted for the production of isotopes of a superheavy nucleus with charge number \(Z=112\) in the \((2-5)n\)-evaporation channels of the complete fusion reactions \(^{48}\)Ca+\(^{233,235}\)U for future experiments. The calculated production cross section of the \(^{277}\)Cn isotope in the hot fusion reaction \(^{48}\)Ca+\(^{233}\)U is compared with the experimental one in the cold fusion reaction \(^{70}\)Zn+\(^{208}\)Pb. The strong correlation between the fusion probability and asymmetry in the entrance reaction channel is revealed. The possibility of filling the gap between the isotopes of superheavy nuclei with \(Z=112\) produced in cold and hot fusion reactions is indicated.

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This manuscript has no associated data or the data will not be deposited. [Authors’ comment: Any data that support the ndings of this study are included within the article.]

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Acknowledgements

The work of GGA and NVA was supported by the Ministry of Science and Higher Education of the Russian Federation (contract 075-10-2020-117). MK was co-financed by the National Science Centre under contract no. UMO-2013/08/M/ST2/00257 (LEA-COPIGAL).

Author information

Authors and Affiliations

  1. Department of Physics and Institute of Physics and Applied Physics, Yonsei University, Seoul, 03722, Korea

    Juhee Hong

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

    G. G. Adamian & N. V. Antonenko

  3. Tomsk Polytechnic University, 634050, Tomsk, Russia

    N. V. Antonenko

  4. National Centre for Nuclear Research, 02-093, Warsaw, Poland

    M. Kowal

  5. Institute of Physics, University of Zielona Góra, 65-516, Zielona Gora, Poland

    P. Jachimowicz

Authors
  1. Juhee Hong
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  2. G. G. Adamian
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  3. N. V. Antonenko
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  4. M. Kowal
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  5. P. Jachimowicz
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Correspondence to G. G. Adamian.

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Communicated by Alexis Diaz-Torres.

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Hong, J., Adamian, G.G., Antonenko, N.V. et al. Hot and cold fusion reactions leading to the same superheavy evaporation residue. Eur. Phys. J. A 58, 180 (2022). https://doi.org/10.1140/epja/s10050-022-00826-3

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