Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions
Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions
The M\"uller-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.
Azwinndini Muronga
物理学
Azwinndini Muronga.Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions[EB/OL].(2001-04-21)[2025-08-02].https://arxiv.org/abs/nucl-th/0104064.点此复制
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