Different coalescence sources of light nucleus production in Au-Au collisions at <inline-formula><tex-math id="M1">\begin{document}${ \sqrt{\boldsymbol s_{\boldsymbol N\boldsymbol N}}=\bf 3 }$\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/7fbf936f-8cf8-4ca4-bfce-9ab11d1765e8/CPC-2023-0434_M1.jpg"/><graphic specific-use="print" xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/7fbf936f-8cf8-4ca4-bfce-9ab11d1765e8/CPC-2023-0434_M1.png"/></alternatives></inline-formula> GeV -

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