Nilsson parameters κ and μ in relativistic mean field models

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Abstract

Nilsson parameters κ and μ have been studied in the framework of relativistic mean field (RMF) models. They are used to investigate the reason why RMF models give a relatively good prediction of the spin-orbit splitting but fail to reproduce the placement of the states with different orbital angular momenta. Instead of the relatively small effective mass M*, the independence of M* from the angular momentum l is found to be the reason.

Original languageEnglish
Article number034312
JournalPhysical Review C - Nuclear Physics
Volume71
Issue number3
DOIs
Publication statusPublished - 1 Jan 2005

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