\begin{document}$P_{\rm eff}-T_{\rm eff}$\end{document} and \begin{document}$T_{\rm eff}-S$\end{document} diagrams are obtained. The coexistent curve and the latent heat of phase transition for this system are also investigated. Furthermore, we analyze the effect of parameters (the state parameter ω and the ratio of two horizon radii \begin{document}$ x=\it{r_{+}} $\end{document}/\begin{document}$ \it{r_{c}} $\end{document}) on the two-phase coexistence region boundary. The results indicate that the phase transition in C-dSSQ spacetime is analogous to that in a van der Waals fluid (vdw) system, which is determined by the electrical potential at the horizon. These results are helpful for understanding the basic properties of black holes and are also of great value for the establishment of quantum gravity."> Continuous phase transition of the de Sitter spacetime with charged black holes and cloud of strings and quintessence -
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