\begin{document}$ ^{40,48} $\end{document}Ca+\begin{document}$ ^{124} $\end{document}Sn and \begin{document}$ ^{64} $\end{document}Ni+\begin{document}$ ^{130} $\end{document}Te based on the DNS model+GEMINI++ are calculated and compared with experimental data. The calculated results reproduce experimental data. The cross sections of fusion-evaporation, fragmentation, and multinucleon transfer reactions in the \begin{document}$ 40 \leq Z \leq 60 $\end{document} region are also provided in this paper. The results show that in the \begin{document}$ 40 \leq Z \leq 60 $\end{document} region, fusion-evaporation and fragmentation reactions have good results in the relatively proton-rich region, but in the extreme proton-deficient region, the MNT reaction is still promising for synthesizing proton-rich nuclei."> Possibilities of synthesizing new proton-rich nuclei with 40 ≤ <i>Z</i> ≤ 60 using multinucleon transfer reactions -
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