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Superheavy nuclei in selfconsistent nuclear calculations

K. Rutz·M. Bender·T. Buervenich·T. Schilling·P. -G. Reinhard·J. A. Maruhn·W. Greiner
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Abstract

The shell structure of superheavy nuclei is investigated within various parametrizations of relativistic and nonrelativistic nuclear mean field models. The heaviest known even-even nucleus 264Hs is used as a benchmark to estimate the predictive value of the models. From that starting point, doubly magic spherical nuclei are searched in the region Z=110-140 and N=134-298. They are found at (Z=114, N=184), (Z=120, N=172), or at (Z=126, N=184), depending on the parametrization.

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K. Rutz, M. Bender, T. Buervenich, T. Schilling, P. -G. Reinhard, J. A. Maruhn, W. Greiner. 1996-10-23. Superheavy nuclei in selfconsistent nuclear calculations. https://doi.org/10.1103/physrevc.56.238

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