Abstract
An effective $\ensuremath{\alpha}$-particle equation is derived for cases where an $\ensuremath{\alpha}$ particle is bound to a doubly magic nucleus. As an example, we consider $^{212}\mathrm{Po}$ with the $\ensuremath{\alpha}$ on top of the $^{208}\mathrm{Pb}$ core. We consider the core nucleus infinitely heavy, so that the $\ensuremath{\alpha}$ particle moves with respect to a fixed center; that is, recoil effects are neglected. The fully quantal solution of the problem is discussed. The approach is inspired by the Tohsaki-Horiuchi-Schuck-R\"opke wave function concept that has been successfully applied to light nuclei. Shell-model calculations are improved by including four-particle ($\ensuremath{\alpha}$-like) correlations that are of relevance when the matter density becomes low. In the region where the $\ensuremath{\alpha}$-like cluster penetrates the core nucleus, the intrinsic bound-state wave function transforms at a critical density into an unbound four-nucleon shell-model state. Exploratory calculations for $^{212}\mathrm{Po}$ are presented. Such preformed cluster states are very difficult to describe with shell-model calculations. Reasons for the different physics behavior of an $\ensuremath{\alpha}$-like cluster with respect to a deuteron-like cluster are discussed.
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