Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter

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dc.creatorNavarra, F.
dc.creatorOrnik, U.
dc.date1994-12-15
dc.date.accessioned2026-07-07T05:41:24Z
dc.date.available2026-07-07T05:41:24Z
dc.descriptionThe 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.
dc.descriptiontalk 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
dc.identifierhttps://arxiv.org/abs/nucl-th/9412024
dc.identifierhttp://arxiv.org/abs/nucl-th/9412024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82558
dc.subjectNuclear Theory
dc.titleHydrodynamic Evolution of Chirally Symmetric Nuclear Matter
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