l4: the navier-stokes equations iii: turbulence and non- newtonian

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L4: The Navier-Stokes equations III: Turbulence and Non-Newtonian Prof. Sauro Succi

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L4: The Navier-Stokes equations III: Turbulence and Non- Newtonian. Prof. Sauro Succi. Turbulence. Turbulence modeling. Effects of small (unresolved) scales o n large (resolved) ones. Energy Cascade. Turbulent energy spectrum: broad and gapless!. Turbulence. Kolmogorov length. - PowerPoint PPT Presentation

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Page 1: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

L4: The Navier-Stokes equations III:Turbulence and Non-Newtonian

Prof. Sauro Succi

Page 2: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence

Page 3: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence modeling

Effects of small (unresolved) scaleson large (resolved) ones

Page 4: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Energy Cascade

Page 5: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulent energy spectrum: broad and gapless!

Page 6: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence

• Kolmogorov length

Page 7: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence

• Kolmogorov length

Faucet, Re=10^4, DOF=10^9,Work=10^12 Car , Re=10^6, DOF=10^14,Geo , Re=10^9, DOF=10^20Astro , Re=10^10,DOF=10^22,Work=10^30

Page 8: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Why is Reynolds so large?

Page 9: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Transition to turbuence

Page 10: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Small and Large Eddies

Page 11: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence: NO scale separation

Small eddies are swept away by large eddies (Advection)Large eddies experience random collisions from small ones (Diffusion)

Brownian motion? NO! Advection/Diffusion is scale-dependent

Dissipative: No Hamiltonian, no standard statistical ensembles

Non-gaussian fluctuations, intermittency,bursts, rare events

Page 12: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Turbulence Cost

Memory CPU

Page 13: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Modeling vs Simulation

Eddy size

Direct Numerical Simulation (DNS)

All significantly excited scales of motion are computed - WORK = O(R3)

Reynolds Averaged Navier-Stokes (RANS)

All scales of motion are described by semi-empirical models

Large Eddy Simulation (LES)

D (grid size) All eddies larger than grid size are computed

Very Large Eddy Simulation (VLES)

Dissipative eddies Inertial range eddies Anisotropic eddiesOnly statistically anisotropic eddies outside the Kolmogorov range are computed

Theory/Model ComputeApproaches:

All CR’s

All-sim’s

Least-computing Multiscale

Principle of Least-Computing!

Page 14: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Complex Fluids

Page 15: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Beyond NSE

Strong gradients: molecular details

Small volumes, large S/V: molecular

Internal structure: complex rheology

Page 16: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Non-Newtonian Fluids

Internal structure: complex rheology

Local, Non-linearNon-localTensor.....

Page 17: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Hydrophobicity: slip flow

Page 18: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Constitutive Relation

Constitutive: sigma=A+B*S^n

Newton: A=0,n=1Yield-Stress A>0n>1 shear-thickening (paints)n<1 shear-thinning (blood,ketch-up…)

Page 19: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian
Page 20: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Boundary Conditions

Periodic: (Free-flows)

Non-slip: zero velocity (Solid walls)

Prescribed pressure/density,Zero velocity: (Open flows)

Moving Boundaries (Pistons, bioflows..)

Page 21: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

End of Lecture 3

Page 22: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Multiscale allies: Universality & Forgiveness

Large Kn allow large Dx and dt

Page 23: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Weak departure from local equilibrium (herd effect)

From Boltzmann to Navier-Stokes: weak non-equilibrium

T

n=n(r,t) u=u(r,t)T=T(r,t)

Order params:

Page 24: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

The evershifting battle: stream and collide

Macro field

Page 25: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Macroscopic persistence: the coherence length

a>1/2a=1/2a=3/4

Below l_c microphysics takes over

weak-> strong

Coupling strength

Page 26: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

(Turbulence)

(Compressibility)

How big is g? Turbulence

Reynolds ~ Length/molecular mean free path!

Page 27: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Bernouilli

Page 28: L4: The  Navier-Stokes equations  III: Turbulence  and Non- Newtonian

Clebsch representation