Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions
| dc.creator | Muronga, Azwinndini | |
| dc.date | 2001-04-21 | |
| dc.date | 2002-01-26 | |
| dc.date.accessioned | 2026-07-07T11:32:36Z | |
| dc.date.available | 2026-07-07T11:32:36Z | |
| dc.description | The Müller-Israel-Stewart second order theory of relativistic imperfect fluids based on Grad's moment method is used to study the expansion of hot matter produced in ultra-relativistic heavy ion collisions. The temperature evolution is investigated in the framework of the Bjorken boost-invariant scaling limit. The results of these second-order theories are compared to those of first-order theories due to Eckart and to Landau and Lifshitz and those of zeroth order (perfect fluid) due to Euler. | |
| dc.description | 5 pages, 4 figures, size of y-axis tick marks for Figs. 3 and 4 fixed | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0104064 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0104064 | |
| dc.identifier | Phys.Rev.Lett.88:062302,2002; Erratum-ibid.89:159901,2002 | |
| dc.identifier | doi:10.1103/PhysRevLett.88.062302 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197648 | |
| dc.subject | Nuclear Theory | |
| dc.title | Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions | |
| dc.type | text |