M. Kozhevnikova and Yu. B. Ivanov
We present results of simulations of light-nuclei production in relativistic heavy-ion collisions within the updated Three-fluid Hydrodynamics-based Event Simulator Extended by UrQMD (ultrarelativistic quantum molecular dynamics) final State interactions (theseus). The simulations were performed for Pb + Pb and Au + Au collisions in the collision energy range of √sNN = 6.4–19.6 GeV. The light-nuclei production is treated within the thermodynamical approach on an equal basis with hadrons. The only additional parameter related to the light nuclei is the energy density of late freeze-out that imitates the afterburner stage of the collision because the light nuclei do not participate in the UrQMD evolution. This parameter is fixed from the condition of the best reproduction of the proton transverse-momentum spectrum after the UrQMD afterburner by that at the late freeze-out. The updated theseus results in an imperfect but reasonable reproduction of data on bulk observables of the light nuclei, especially their functional dependence on the collision energy and light-nucleus mass. Various ratios, d/p, t/p , t/d and N(t)×N(p)/N²(d), are also considered. The directed flow of light nuclei turns out to be more involved. Apparently, it requires explicit treatment of the afterburner evolution of light nuclei that violates the kinetic equilibrium. Imperfect reproduction of the light-nuclei data leaves room for medium effects in produced light nuclei.