Nuclear $α$-cluster structures from valence-space microscopic cluster model

Abstract

Alpha clustering is an important dynamic in nuclear physics, with growing interest to its study in heavy nuclei in recent years. Theoretically, the microscopic cluster models taking nucleons as relevant degrees of freedom have been widely used to study $α$-cluster structures in light nuclei. However, a straightforward application on same footing in heavy nuclei is obstructed by the complexity of handling numerous nucleons. As a simplified alternative, the macroscopic cluster models built upon cluster degrees of freedom are usually employed in heavy nuclei, though these approaches typically lose several critical structural details. In this work, we propose to study the $α$-cluster structures within the framework of valence-space microscopic cluster model (VS-MCM), which is a hybrid between microscopic and macroscopic cluster models and inherits features from both models, making it capable to investigate the $α$-cluster structures in heavy nuclei from a relatively microscopic viewpoint. In VS-MCM, the valence $α$ clusters are described by antisymmetrized microscopic wave functions, with single-particle orbits in core nuclei removed systematically from the model space via the Pauli projection to simulate the antisymmetrization between $α$ clusters and doubly magic cores. As a proof of principle, we apply the VS-MCM to study the $α$-cluster structures in ${}^{20}$Ne and ${}^{44}$Ti at first, with the theoretical energy levels of the $K^π=0_1^{\pm}$ bands for ${}^{20}$Ne and ${}^{44}$Ti showing reasonable agreement with experimental data. These calculations lay the foundation for future applications of VS-MCM in general cluster structures across the nuclide chart, where more $α$ clusters and valence nucleons can exist outside the heavy doubly magic core, opening new avenues to study the $α$ and cluster decays in heavy nuclei microscopically.