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Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter

F. Navarra·U. Ornik
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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.

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F. Navarra, U. Ornik. 1994-12-15. Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter. https://arxiv.org/abs/nucl-th/9412024

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