Resolution of hyper-triton chemical freeze-out puzzle in high energy nuclear collisions
arXiv:2007.07376 · doi:10.1140/epja/s10050-021-00370-6
Abstract
The recently developed hadron resonance gas model with multicomponent hard-core repulsion is used to address and resolve the long standing problem to describe the light nuclear cluster multiplicities including the hyper-triton measured by the STAR Collaboration, known as the hyper-triton chemical freeze-out puzzle. An unprecedentedly accurate description is obtained for the hadronic and other light nuclear cluster data measured by STAR at the collision energy GeV and by ALICE at TeV. This success is achieved by applying the new strategy of analyzing the light nuclear cluster data and by using the value for the hard-core radius of the (anti-) hyperons found in earlier work. One of the most striking results of the present work is that for the most probable scenario of chemical freeze-out for the STAR energy the obtained parameters allow to simultaneously reproduce the values of the experimental ratios and which were not included in the fit.
arXiv comment12 pages, 5 figures and 4 tables
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