\begin{document}$ A^{*} $\end{document} in terms of cosmological constant Λ: \begin{document}$ A^{*}\propto (0.01360 \sigma/v_{0}+ 0.001751)\Lambda $\end{document}, where σ denotes the initial width of the scalar field and \begin{document}$ v_{0} $\end{document} is the initial position of the scalar field. Notably, we highlight that the slope of this linear relationship depends on the initial configuration of the scalar field."> Critical collapse of massless scalar fields in asymptotically anti-de Sitter spacetime -
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