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We present a summary of the recent results obtained with the novel hadronresonance gas model with the multicomponent hard-core repulsion which isextended to describe the mixtures of hadrons and light (anti-, hyper-)nuclei. Avery accurate description is obtained for the hadronic and the light nucleidata measured by STAR at the collision energy $\sqrt{s_{NN}} =200$ GeV and byALICE at $\sqrt{s_{NN}} =2.76$ TeV. The most striking result discussed here isthat for the most probable chemical freeze-out scenario for the STAR energy thefound parameters allow us to reproduce the values of the experimental ratios$S_3$ and $\overline{S}_3$ without fitting.

Chemical freeze-out of light nuclei in high energy nuclear collisions and resolution of the hyper-triton chemical freeze-out puzzle