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Energy dependence of light (anti)nuclei and (anti)hypertriton production in the Au-Au collision from sNN=5.0\sqrt{s_{\rm{NN}}} =5.0 to $5020$ GeV

Published 5 Mar 2018 in nucl-th and hep-ph | (1803.01547v1)

Abstract: The energy dependence of light (anti)nuclei and (anti)hypertriton production are investigated in central Au-Au collisions from AGS up to LHC energies at midrapidity, using the parton and hadron cascade model (PACIAE) together with the dynamically constrained phase-space coalescence model(DCPC). We find that the yields, yield ratios of the antiparticles to their corresponding particles, the coalescence parameters BAB_A and the strangeness population factor s3s_3 of light (anti)nuclei and (anti)hypertriton strongly depend on the energy. Furthermore, we analyze and discuss the strangeness population factor s3s_3 and the coalescence parameters BAB_A, and find a transition point near by 20 GeV. These results thus suggest the potential usefulness of the s3s_3 and BAB_A of light nuclei production in relativistic heavy-ion collisions as a direct probe of the transition point associated with the QCD critical phenomena. The results from PACIAE+DCPC model are well consistent with experimental data.

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