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Shell evolution at N=20 in the constrained relativistic mean field approach
shell quenching N=20 relativistic mean field theory nuclear deformation
2009/8/14
The shell evolution at N=20, a disappearing neutron magic number observed experimentally in very neutron-rich nuclides, is investigated in the constrained relativistic mean field (RMF) theory. The tr...
The Coester Line in Relativistic Mean Field Nuclear Matter
The Coester Line Relativistic Mean Field Nuclear Matter
2010/10/13
The Walecka model contains essentially two parameters that are associated with the Lorentz scalar (S) and vector (V ) interactions. These parameters are related to a two-body interaction consisting of...