\begin{document}$ Q^{2} $\end{document} using the parametrization \begin{document}$ F_{2}(x,Q^{2}) $\end{document}and the nuclear modification factors obtained from the Khanpour-Soleymaninia-Atashbar-Spiesberger-Guzey model. The CT18 gluon distribution is used for the baseline proton gluon density at \begin{document}$ Q_{0}^{2}=1.69\; {\rm{GeV}}^2 $\end{document}. We discuss the behavior of the gluon densities in the next-to-leading order and the next-to-next-to-leading order approximations at the initial scale \begin{document}$ Q_{0}^{2} $\end{document}, as well as the modifications due to the nonlinear corrections. We find that the QCD nonlinear corrections are more significant for the next-to-leading order accuracy than the next-to-next-to-leading order for light and heavy nuclei. The results of the nonlinear GLR-MQ evolution equation are similar to those obtained with the Rausch-Guzey-Klasen gluon upward and downward evolutions within the uncertainties. The magnitude of the gluon distribution with the nonlinear corrections increases with a decrease in x and an increase in atomic number A."> Nonlinear corrections for the nuclear gluon distribution in <i>eA</i> processes -
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