\begin{document}$ H^{2} $\end{document} in the early universe and to H in the present and late universe, where H depicts the Hubble parameter. Consequently, we obtain the solutions \begin{document}$ a(t)\propto {\rm e}^{\alpha t/3} $\end{document} and \begin{document}$ a(t)\propto t^{1/2} $\end{document} for the early universe and solutions \begin{document}$ a(t)\propto t^{\delta} $\end{document} and \begin{document}$ a(t)\propto {\rm e}^{Ht} $\end{document} for the present and late universe, respectively, where \begin{document}$ \alpha $\end{document} and \begin{document}$ \delta $\end{document} are the parameters. Finally, we obtain and analyze two important thermodynamic properties for the present model."> Cosmological scenario based on particle creation and holographic equipartition -
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