Spectroscopic factors of resonance states with the Gamow shell model
M.R. Xie, J.G. Li, N. Michel, H.H. Li, W. Zuo

TL;DR
This paper investigates resonance state spectroscopic factors in light nuclei using the Gamow shell model, demonstrating its superior accuracy in reproducing resonance states and wave function asymptotes compared to other methods.
Contribution
It introduces a comprehensive GSM approach that accurately incorporates continuum coupling and configuration mixing for resonance states, validated against other models and experimental data.
Findings
GSM reproduces low-lying resonance states more accurately than NCSM.
GSM effectively models wave function asymptotes for resonance states.
Systematic calculations of overlap functions align well with experimental data.
Abstract
We provide an investigation of the spectroscopic factor of resonance states in nuclei, utilizing the Gamow shell model (GSM). Within the GSM, the configuration mixing is taken into account exactly with the shell model framework, and the continuum coupling is addressed via the complex-energy Berggren ensemble, which treats bound, resonance, and non-resonant continuum single-particle states on an equal footing. As a result, both the configuration mixing and continuum coupling are meticulously considered in the GSM. We first calculate the low-lying states of helium isotopes and isotones with the GSM, and the results are compared with that of \textit{ab initio} no-core shell model (NCSM) calculations. The results indicate that GSM can reproduce the low-lying resonance states more accurately than the no-core shell model. Following this, we delve into the spectroscopic factors of the…
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