Abstract
The expansion of the fireball created in Au-Au collisions at GeV and Pb-Pb collisions at TeV is modelled using relativistic viscous hydrodynamics. The experimentally observed interferometry radii are well reproduced. Additional pre-equilibrium flow slightly improves the results for the lower energies studied.
- Received 29 December 2010
DOI:https://doi.org/10.1103/PhysRevC.83.044910
©2011 American Physical Society