\begin{document}$ 5 $\end{document}- and \begin{document}$ 6 $\end{document}-dimensional Einstein-Maxwell-Gauss-Bonnet-de Sitter black holes. Our numerical results show that the higher derivative term plays a different role in the \begin{document}$ d = 5 $\end{document} case than it does in the \begin{document}$ d = 6 $\end{document} case. For \begin{document}$ d = 5 $\end{document}, the SCC violation region increases as the strength of the higher derivative term increases. For \begin{document}$ d = 6 $\end{document}, the SCC violation region first increases and then decreases as the higher derivative correction becomes stronger, and SCC can always be restored for a black hole with a fixed charge ratio when the higher derivative correction is strong enough. Finally, we find that the \begin{document}$ C^{2} $\end{document} version of SCC is respected in the \begin{document}$ d = 6 $\end{document} case, but can be violated in some near-extremal regimes in the \begin{document}$ d = 5 $\end{document} case."> Strong cosmic censorship for a scalar field in an Einstein-Maxwell-Gauss-Bonnet-de Sitter black hole -
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