\begin{document}$\mu=306~ \mathrm{MeV}$\end{document} and \begin{document}$\mu=309 ~\mathrm{MeV}$\end{document}. Our results show that the system could be trapped in the metastable state for a long time as long as the temperature is between the metastable region characterized by the up and low spinodal lines. Moreover, the surface tension at criticality will rise to approximately \begin{document}$4~ \mathrm{MeV/fm^2}$\end{document} when the chemical potential is very high. Such a small surface tension value would favor a mixed phase in the cores of compact stars and may have an important implication in astrophysics."> Bubble nucleation in the two-flavor quark-meson model -
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