Abstract:Due to large pressure gradients at early times, standard hydrodynamic model simulations of relativistic heavyion collisions do not become reliable until O(1) fm/c after the collision. To address this one often introduces a pre-hydrodynamic stage that models the early evolution microscopically, typically as a conformal, weakly interacting gas. In such an approach the transition from the pre-hydrodynamic to the hydrodynamic stage is discontinuous, introducing considerable theoretical model ambiguity. Alternative… Show more
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