Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter
Nuclear Theory
2007-05-23 v1
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.
Keywords
Cite
@article{arxiv.nucl-th/9412024,
title = {Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter},
author = {F. Navarra and U. Ornik},
journal= {arXiv preprint arXiv:nucl-th/9412024},
year = {2007}
}
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