Superheavy nuclei in selfconsistent nuclear calculations

Preprint

23 October 1996

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.nucl-th/9610032

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.

Keywords

VARIOUS PARAMETRIZATIONS
SELFCONSISTENT NUCLEAR
NUCLEAR CALCULATIONS
SUPERHEAVY NUCLEI
SPHERICAL NUCLEI
HEAVIEST KNOWN
NUCLEUS 264HS

All Related Versions

Version 1, 1996-10-23, ArXiv
Published version: Physical Review C, 56 (1), 238.

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