Dissipative hydrodynamics for viscous relativistic fluids
| dc.creator | Heinz, Ulrich W. | |
| dc.creator | Song, Huichao | |
| dc.creator | Chaudhuri, Asis K. | |
| dc.date | 2005-10-04 | |
| dc.date.accessioned | 2026-07-07T11:28:19Z | |
| dc.date.available | 2026-07-07T11:28:19Z | |
| dc.description | Explicit equations are given for describing the space-time evolution of non-ideal (viscous) relativistic fluids undergoing boost-invariant longitudinal and arbitrary transverse expansion. The equations are derived from the second-order Israel-Stewart approach which ensures causal evolution. Both azimuthally symmetric (1+1)-dimensional and non-symmetric (2+1)-dimensional transverse expansion are discussed. The latter provides the formal basis for the hydrodynamic computation of elliptic flow in relativistic heavy-ion collisions including dissipative effects. | |
| dc.description | 12 pages, no figures. Submitted to Physical Review C | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0510014 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0510014 | |
| dc.identifier | Phys.Rev.C73:034904,2006 | |
| dc.identifier | doi:10.1103/PhysRevC.73.034904 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/196406 | |
| dc.subject | Nuclear Theory | |
| dc.title | Dissipative hydrodynamics for viscous relativistic fluids | |
| dc.type | text |