Light Nuclei Production in Au+Au Collisions at = 3 GeV from the STAR experiment
Hui Liu (for the STAR Collaboration)🇨🇳
Light nuclei production is expected to be sensitive to baryon density fluctuations and can be used to probe the signatures of QCD critical point and/or a first-order phase transition in heavy-ion collisions. In this proceedings, we present the spectra and yields of protons () and light nuclei (, , , ) in Au+Au collisions at = 3 GeV by the STAR experiment. Finally, it is found that the kinetic freeze-out dynamics (temperature average radial flow velocity ) at 3 GeV extracted with the blast-wave model deviate from the trends at high energies ( = 7.7 - 200 GeV), indicating a different medium equation of state.