QCD at high density: Equation of state for nuclear collisions and neutron stars [CL]

http://arxiv.org/abs/1809.02000


A unified chiral mean field approach is presented for QCD thermodynamics in a wide range of temperatures and densities. The model simultaneously gives a satisfactory description of lattice QCD thermodynamics and fulfills nuclear matter and astrophysical constraints. The resulting equation of state can be incorporated in relativistic fluid-dynamical simulations of heavy-ion collisions and neutron stars mergers. Access to different regions of the QCD phase diagram can be obtained in simulations of heavy-ion data and observations of neutron star mergers.

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A. Motornenko, V. Vovchenko, J. Steinheimer, et. al.
Fri, 7 Sep 18
23/65

Comments: 4 pages, 2 figures. Contribution to the Quark Matter 2018 conference proceedings