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A basic introduction to the nuclear shell model is presented, with illustrative explanations of shell-model concepts and procedures. All details of many-body theories are avoided. First, we explain how magic numbers and shell structures appear from fundamental properties of nuclei such as the short-range attractive interaction and density saturation. Some concepts needed to understand the shell model are explained from scratch. The process of the shell model calculation is sketched also in a visual way. After the introduction, one of the recent topics, the evolution of shell structure in exotic nuclei, is briefly discussed, mentioning the importance of the tensor force.
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