Light Nuclei Production in Au+Au Collisions at = 5-200 GeV from JAM model
arXiv:1909.09304 · doi:10.1016/j.physletb.2020.135452
Abstract
Light nuclei production is sensitive to the baryon density fluctuations and can be used to probe the QCD phase transition in relativistic heavy-ion collisions. In this work, we studied the production of proton, deuteron, triton in central Au+Au collisions at = 5, 7.7, 11.5, 14.5, 19.6, 27, 39, 54.4, 62.4 and 200 GeV from a transport model (JAM). Based on the coalescence production of light nuclei, we calculated the energy dependence of rapidity density and particle ratios (, , and ). More importantly, the yield ratio , which is sensitive to the neutron density fluctuations, shows a flat energy dependence and cannot describe the non-monotonic trend observed by the STAR experiment. Based on the nucleon coalescence, this work can provide constraint and reference to search for the QCD critical point and/or first order phase transition with light nuclei production in future heavy-ion collision experiments.
5 pages, 4 figures
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- QFT treatment of a bound state in a thermal gas
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- Measurements on the production and properties of light hypernuclei at STAR
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