Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter

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The equation of state of the linear sigma model in the mean field approximation is used as input in a relativistic hydrodynamical numerical routine. Longitudinal and transverse energy distributions are calculated and compared with those obtained from the QHD-I equation of state.
talk presented at the 5$^{th}$ workshop on hadronic interactions, Sao Paulo, 1-3 Dec. 1994. 6 pages, figures included. Format: compressed and uuencoded postscript file

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