Comparing the first and second order theories of relativistic dissipative fluid dynamics using the 1+1 dimensional relativistic flux corrected transport algorithm
| dc.creator | Molnar, Etele | |
| dc.date | 2008-07-03 | |
| dc.date | 2009-02-15 | |
| dc.date.accessioned | 2026-07-07T12:55:07Z | |
| dc.date.available | 2026-07-07T12:55:07Z | |
| dc.description | Focusing on the numerical aspects and accuracy we study a class of bulk viscosity driven expansion scenarios using the relativistic Navier-Stokes and truncated Israel-Stewart form of the equations of relativistic dissipative fluids in 1+1 dimensions. The numerical calculations of conservation and transport equations are performed using the numerical framework of flux corrected transport. We show that the results of the Israel-Stewart causal fluid dynamics are numerically much more stable and smoother than the results of the standard relativistic Navier-Stokes equations. | |
| dc.description | 16 pages, 17 figures; revised version with added references and updated text and figures; to be published in EPJ C | |
| dc.identifier | https://arxiv.org/abs/0807.0544 | |
| dc.identifier | http://arxiv.org/abs/0807.0544 | |
| dc.identifier | Eur.Phys.J.C60:413-429,2009 | |
| dc.identifier | doi:10.1140/epjc/s10052-009-0927-0 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/224159 | |
| dc.subject | Nuclear Theory | |
| dc.title | Comparing the first and second order theories of relativistic dissipative fluid dynamics using the 1+1 dimensional relativistic flux corrected transport algorithm | |
| dc.type | text |