Shell model structure of proxy-SU(3) pairs of orbitals

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作者
Dennis Bonatsos
Hadi Sobhani
Hassan Hassanabadi
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[1] National Centre for Scientific Research “Demokritos”,Institute of Nuclear and Particle Physics
[2] Shahrood University of Technology,Faculty of Physics
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The Nilsson orbitals used in the substitutions occurring in the proxy-SU(3) scheme, which are the orbitals bearing the maximum value of total angular momentum in each shell, have an extremely simple structure in the shell model basis |NljΩ⟩\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$|N l j \Omega \rangle $$\end{document}, with each Nilsson orbital corresponding to a single-shell model eigenvector. This simple structure is valid at all deformations for these orbitals, while in other orbitals it is valid only at small deformations. Nilsson 0[110] pairs are found to correspond to |1110⟩\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$|1 1 1 0\rangle $$\end{document} pairs in the spherical shell model basis, paving the way for using the proxy-SU(3) approximation within the shell model.
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