Bayesian analysis for constraining the equation of state of asymmetric nuclear matter

The equation of state of nuclear matter plays a crucial role in understanding the properties of neutron stars and heavy-ion collisions. However, due to the complexities of nuclear interactions, accurately constraining the EoS remains a challenging task. We present results of combining Bayesian analysis of the transport model simulations and the single particle spectra, and particle ratios from the Ca+Ni and Ca+Sn collisions at E/A=56 and 140 MeV performed at the National Superconducting Cyclotron Laboratory.