arXiv · nucl-th/0510092
Hubble-like flows in relativistic heavy-ion collisions
Abstract
We study the dynamical appearance of scaling solutions in relativistic hydrodynamics. The phase transition effects are included through the temperature dependent sound velocity. If a pre-equilibrium transverse flow is included in the initial conditions, then it may reach the form of the asymptotic Hubble flow, r/t, in short evolution times, 7-15 fm. The numerical solutions are found to support to the freeze-out models (Blast-Wave, Buda-Lund, Cracow).
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M. Chojnacki. 2006-01-30. Hubble-like flows in relativistic heavy-ion collisions. https://doi.org/10.1556/aph.27.2006.2-3.33
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