dorsal/arxiv
View SchemaHydrodynamic Evolution of Chirally Symmetric Nuclear Matter
| Authors | F. Navarra, U. Ornik |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9412024 |
| URL | https://arxiv.org/abs/nucl-th/9412024 |
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.
{
"annotation_id": "617f9039-ce0f-496d-807c-015339f8b098",
"date_created": "2026-03-02T18:00:15.528000Z",
"date_modified": "2026-03-02T18:00:15.528000Z",
"file_hash": "8c2249d141d44133bf23ae6de7f924c36e6efdd72a25465fdc72e92f4d37dd03",
"private": false,
"record": {
"abstract": "The equation of state of the linear sigma model in the mean field\napproximation is used as input in a relativistic hydrodynamical numerical\nroutine. Longitudinal and transverse energy distributions are calculated and\ncompared with those obtained from the QHD-I equation of state.",
"arxiv_id": "nucl-th/9412024",
"authors": [
"F. Navarra",
"U. Ornik"
],
"categories": [
"nucl-th"
],
"title": "Hydrodynamic Evolution of Chirally Symmetric Nuclear Matter",
"url": "https://arxiv.org/abs/nucl-th/9412024"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "c2c6819e-0e2b-4bf3-bc61-9c6e33932b07",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}