\begin{document}$ {\mathrm{iEBE-VISHNU}}$\end{document} under TRENTo initial conditions to study the collective flow and fluid behavior in p/d/3He+Au collisions. With fine-tuned parameters, \begin{document}$ {\mathrm{iEBE-VISHNU}}$\end{document} can describe the \begin{document}$ v_2(p_T) $\end{document} and \begin{document}$ v_3(p_T) $\end{document} data from the PHENIX and STAR collaborations. However, for certain parameter sets with initial sub-nucleon fluctuations, the hydrodynamic simulations already go beyond their limits with an average Knudsen number \begin{document}$ \langle K_n \rangle $\end{document} clearly larger than unity. Our calculations demonstrate that, for a meaningful evaluation of the fluid behavior in small systems, model simulations must also pay attention to the validity range of hydrodynamics."> Collective flow and fluid behavior in <i>p</i>/<i>d</i>/<sup>3</sup>He+Au collisions at <inline-formula><tex-math id="M1">\begin{document}${ \sqrt{\boldsymbol s_{\boldsymbol NN}} \bf = 200}$\end{document}</tex-math><alternatives><graphic specific-use="online" xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/96fe2b3d-2966-40cd-9938-271aba3a9203/CPC-2024-0342_M1.jpg"/><graphic specific-use="print" xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/96fe2b3d-2966-40cd-9938-271aba3a9203/CPC-2024-0342_M1.png"/></alternatives></inline-formula> GeV -
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