Relaxation-time approximation and relativistic third-order viscous hydrodynamics from kinetic theory
arXiv:1407.0837 · doi:10.1016/j.nuclphysa.2014.08.035
Abstract
Using the iterative solution of Boltzmann equation in the relaxation-time approximation, the derivation of a third-order evolution equation for shear stress tensor is presented. To this end we first derive the expression for viscous corrections to the phase-space distribution function, , up to second-order in derivative expansion. The expression for obtained in this method does not lead to violation of the experimentally observed scaling of the femtoscopic radii, as opposed to the widely used Grad's 14-moment approximation. Subsequently, we present the derivation of a third-order viscous evolution equation and demonstrate the significance of this derivation within one-dimensional scaling expansion. We show that results obtained using third-order evolution equations are in excellent accordance with the exact solution of Boltzmann equation as well as with transport results.
4 pages, 2 figures, Flash Talk given at Quark Matter 2014, Darmstadt, Germany
References in corpus (4)
- Dissipative relativistic fluid dynamics: a new way to derive the equations of motion from kinetic theory
- Transport rates and momentum isotropization of gluon matter in ultrarelativistic heavy-ion collisions
- Constraining relativistic viscous hydrodynamical evolution
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Cited by in corpus (5)
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- Gradient expansion for anisotropic hydrodynamics
- Non-conformal evolution of magnetic fields during reheating
- Formulation of relativistic dissipative fluid dynamics and its applications in heavy-ion collisions