Direct numerical simulation of the turbulent flows of power-law fluids in a circular pipe
A.A. Gavrilov1В and V.Ya. Rudyak2
1Kutateladze Institute of Thermophysics SB RAS, Novosibirsk, Russia
2Novosibirsk State University of Architecture and Civil Engineering,В Novosibirsk, Russia
E-mail: valery.rudyak@mail.ru
Keywords: non-Newtonian fluids, power-law fluids, turbulent flows, direct numerical simulation, flow in a circu-lar pipe, turbulence anisotropy, viscosity pulsations
Pages: 473–486
Abstract
Fully developed turbulent pipe flows of power-law fluids are studied by means of direct numerical simulation. Two series of calculations at generalised Reynolds numbers of approximately 10000 and 20000 were carried out. Five different power law indexes n from 0.4 to 1 were considered. The distributions of components of Reynolds stress tensor, averaged viscosity, viscosity fluctuations, and measures of turbulent anisotropy are presented. The friction coefficient predicted by the simulations is in a good agreement with the correlation obtained from experiment. Flows of power-law fluids exhibit stronger anisotropy of the Reynolds stress tensor compared with the flow of Newtonian fluid. The turbulence anisotropy becomes more significant with the decreasing flow index n. An increase in apparent viscosity away from the wall leads to the damping of the wall-normal velocity pulsations. The suppression of the turbulent energy redistribution between the Reynolds stress tensor components observed in the simulations leads to a strong domination of the axial velocity pulsations. The damping of wall-normal velocity pulsations leads to a reduction of the fluctuating transport of momentum from the core toward the wall, which explains the effect of drag reduction.
DOI: 10.1134/S0869864316040016
|
