Evolution of Hot, Dissipative Quark Matter in Relativistic Nuclear Collisions
arXiv:nucl-th/0407114
Abstract
Non-ideal fluid dynamics with cylindrical symmetry in transverse direction and longitudinal scaling flow is employed to simulate the space-time evolution of the quark-gluon plasma produced in heavy-ion collisions at RHIC energies. The dynamical expansion is studied as a function of initial energy density and initial time. A causal theory of dissipative fluid dynamics is used instead of the standard theories which are acausal. We compute the parton momentum spectra and HBT radii from two-particle correlation functions. We find that, in non-ideal fluid dynamics, the reduction of the longitudinal pressure due to viscous effects leads to an increase of transverse flow and a decrease of the ratio as compared to the ideal fluid approximation.
arXiv comment25 pages, 5 figures, corrected typos and and minor changes
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