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The aim of this Conference is to bring together physicists working on strong interacting dense matter, QCD phase diagram, ultrarelativistic heavy-ion collisions with astrophysicists working on Compact Stars (from their birth in core-collapse supernovae to their old age as cold radio pulsars including binary merger events) and on related phenomena. A profound theoretical description of these phenomena necessarily involves the equation of state and transport properties of QCD matter that are derived from nonperturbative quantum field theories, many-body physics of strong interacting matter and phenomenological investigations.
