\begin{document}$f(Q, C)$\end{document} gravity, where \begin{document}$Q$\end{document} is the non-metricity scalar and \begin{document}$C$\end{document} represents the boundary term, considering both interacting and non-interacting models. A set of autonomous equations is derived, and solutions are calculated accordingly. We assess the critical points obtained from these equations, identify their characteristic values, and explore the physical interpretation of the phase space for this system. Two types of \begin{document}$f(Q, C)$\end{document} are assumed: \begin{document}$({\rm{i}})$\end{document} \begin{document}$f(Q, C)=Q+\alpha Q+\beta C {\rm{log}}C$\end{document} and \begin{document}$({\rm{ii}})$\end{document} \begin{document}$f(Q, C)=Q+\alpha Q+\frac{\beta}{C}$\end{document}, where \begin{document}$\alpha$\end{document} and \begin{document}$\beta$\end{document} are the parameters. In Model I, we obtain two stable critical points, whereas in Model II, we identify three stable critical points for both interacting and non-interacting models. We examine the behavior of phase space trajectories at every critical point. We calculate the values of the physical parameters for both systems at each critical point, indicating the accelerated expansion of the Universe."> Phase space analysis of interacting and non-interacting models in f(<i>Q</i>, <i>C</i>) gravity -
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