\begin{document}$ sd $\end{document}-shell nuclei. The low-lying spectra of Al isotopes and \begin{document}$ N=8 $\end{document} isotones, together with their mirror nuclei, were calculated, followed by a systematic analysis of the evolution of the mirror energy difference. The results suggest that the large mirror energy difference is mainly caused by the weakly-bound effects and large average occupations of the \begin{document}$ 1s_{1/2} $\end{document} orbit. Lastly, we compare the results of our ab initio calculations with shell model results, elucidating the relationship and coherence between these two models."> <i>Ab initio</i> calculations of mirror energy difference in <i>sd</i>-shell nuclei -
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