Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter

Abstract

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.

Comments: 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