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Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions

Second Order Dissipative Fluid Dynamics for Ultra-Relativistic Nuclear Collisions

来源:Arxiv_logoArxiv
英文摘要

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

10.1103/PhysRevLett.88.062302

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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