Superheavy nuclei in selfconsistent nuclear calculations

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dc.creatorRutz, K.
dc.creatorBender, M.
dc.creatorBuervenich, T.
dc.creatorSchilling, T.
dc.creatorReinhard, P. -G.
dc.creatorMaruhn, J. A.
dc.creatorGreiner, W.
dc.date1996-10-23
dc.date.accessioned2026-07-07T11:36:37Z
dc.date.available2026-07-07T11:36:37Z
dc.descriptionThe 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.
dc.description16 pages RevTeX, 2 tables, 2 low resolution Gif figures (high resolution PostScript versions are available at http://www.th.physik.uni-frankfurt.de/~bender/nucl_struct_publications.html or at ftp://th.physik.uni-frankfurt.de/pub/bender ), submitted to Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9610032
dc.identifierhttp://arxiv.org/abs/nucl-th/9610032
dc.identifierPhys.Rev.C56:238-243,1997
dc.identifierdoi:10.1103/PhysRevC.56.238
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198976
dc.subjectNuclear Theory
dc.titleSuperheavy nuclei in selfconsistent nuclear calculations
dc.typetext

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