Collective flow of light nuclei and hyper-nuclei in Au+Au collisions at √SNN = 3, 14.6, 19.6, 27, and 54.4 GeV using the STAR detectorRishabh SharmaEPJ Web Conf., 276 (2023) 04006DOI: https://doi.org/10.1051/epjconf/202327604006