Stress tensor for non-Newtonian fluid

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SUMMARY

The setup of the stress tensor for non-Newtonian fluids, particularly power law fluids, involves defining shear stress as K(du/dy)^n, where K is the consistency index and n is the flow behavior index. In symmetric pipes or rectangular ducts, the normal stresses are represented by pressure, while other stress components may be zero. For purely viscous non-Newtonian fluids, the viscosity is expressed as a function of the second invariant of the rate of deformation tensor, paralleling the approach used for Newtonian fluids as detailed in "Transport Phenomena" by Bird, Stewart, and Lightfoot.

PREREQUISITES
  • Understanding of non-Newtonian fluid mechanics
  • Familiarity with the power law model for fluid behavior
  • Knowledge of stress tensors and their components
  • Basic principles of fluid dynamics and flow in ducts
NEXT STEPS
  • Study the derivation of the stress tensor for non-Newtonian fluids
  • Explore the application of the second invariant of the rate of deformation tensor
  • Investigate the differences between Newtonian and non-Newtonian fluid behavior
  • Review case studies involving power law fluids in engineering applications
USEFUL FOR

Fluid mechanics engineers, researchers in rheology, and professionals involved in the design of systems handling non-Newtonian fluids will benefit from this discussion.

ccrook
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How does one setup the stress tensor for a non-Newtonian fluid? I know that for any fluid the normals should be the pressure and for a power law fluid the shear stress in the direction of flow is related by K(du/dy)^n. Does this mean that all other components are 0 for a symmetric pipe or rectangular duct?
 
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ccrook said:
How does one setup the stress tensor for a non-Newtonian fluid? I know that for any fluid the normals should be the pressure and for a power law fluid the shear stress in the direction of flow is related by K(du/dy)^n. Does this mean that all other components are 0 for a symmetric pipe or rectangular duct?
For a purely viscous non-Newtonian fluid (not viscoelastic), you use exactly the same form of equation as for a Newtonian fluid (see Bird, Stewart, and Lightfoot), except that you represent the viscosity as a function of the 2nd invariant of the rate of deformation tensor. There is a form of this functionality that gives the same behavior as a power law fluid for simple shear flows.

Chet
 

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