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• W1977351337 endingPage "67" @default.
• W1977351337 startingPage "62" @default.
• W1977351337 abstract "The analysis of quasi-particle spectra in the heaviest A∼250 nuclei with spectroscopic data provides an additional constraint for the choice of effective interaction for the description of superheavy nuclei. It strongly suggests that only the parametrizations which predict Z=120 and N=172 as shell closures are reliable for superheavy nuclei within the relativistic mean field theory. The influence of the central depression in the density distribution of spherical superheavy nuclei on the shell structure is studied. A large central depression produces large shell gaps at Z=120 and N=172. The shell gaps at Z=126 and N=184 are favoured by a flat density distribution in the central part of the nucleus. It is shown that approximate particle number projection (PNP) by means of the Lipkin–Nogami (LN) method removes pairing collapse seen at these gaps in the calculations without PNP." @default.
• W1977351337 created "2016-06-24" @default.
• W1977351337 creator A5008670107 @default.
• W1977351337 date "2006-06-28" @default.
• W1977351337 modified "2023-09-27" @default.
• W1977351337 title "Superheavy nuclei: a relativistic mean field outlook" @default.
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• W1977351337 doi "https://doi.org/10.1088/0031-8949/2006/t125/014" @default.
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