arXiv · 0907.0923
Skyrme-Rpa Description of Spin-Flip M1 Giant Resonance
Abstract
The spin-flip M1 giant resonance is explored in the framework of Random Phase Approximation on the basis of the Skyrme energy functional. A representative set of eight Skyrme parameterizations (SkT6, SkM*, SLy6, SG2, SkO, SkO', SkI4, and SV-bas) is used. Light and heavy, spherical and deformed nuclei ($^{48}$Ca, $^{158}$Gd, $^{208}$Pb, and $^{238}$U) are considered. The calculations show that spin densities play a crucial role in forming the collective shift in the spectrum. The interplay of the collective shift and spin-orbit splitting determines the quality of the description. None of the considered Skyrme parameterizations is able to describe simultaneously the M1 strength distribution in closed-shell and open-shell nuclei. It is found that the problem lies in the relative positions of proton and neutron spin-orbit splitting. Necessity to involve the tensor and isovector spin-orbit interaction is called for.
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P. Vesely, J. Kvasil, V. O. Nesterenko, W. Kleinig, P. -G. Reinhard, V. Yu. Ponomarev. 2009-07-06. Skyrme-Rpa Description of Spin-Flip M1 Giant Resonance. https://doi.org/10.1103/physrevc.80.031302
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