Viscous Compaction Waves Joseph M. Powers and Michael T. Cochran - - PowerPoint PPT Presentation

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Viscous Compaction Waves Joseph M. Powers and Michael T. Cochran University of Notre Dame, Notre Dame, Indiana SIAM Annual Meeting New Orleans, Louisiana 12 July 2005 Compaction Wave Schematic 100 m D ~ 400 m/s u ~ 100 m/s p particles


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SLIDE 1

Viscous Compaction Waves Joseph M. Powers and Michael T. Cochran University of Notre Dame, Notre Dame, Indiana SIAM Annual Meeting New Orleans, Louisiana 12 July 2005

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SLIDE 2

Compaction Wave Schematic

u ~ 100 m/s

p

φ ~ 0.73 φ ~ 0.98

D ~ 400 m/s

s s 100 µm particles

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SLIDE 3

Introduction

  • Heterogeneous energetic solids composed of

100 µm crystals in plastic binder.

  • Engineering length scales on the order of many cm.
  • Macrobehavior (ignition, etc.) strongly linked to

microstructure.

  • Continuum mixture models with non-traditional

constitutive theories needed to capture grain scale physics.

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SLIDE 4

Review

  • Gokhale and Krier, Prog. Energy Combust. Sci.,

1982.

  • Baer and Nunziato, Int. J. Multiphase Flow, 1986.
  • Powers, Stewart, Krier, Combust. Flame, 1990.
  • Saurel and Abgrall, J. Comput. Phys., 1999.
  • Bdzil, et al. Phys. Fluids, 1999, 2001.
  • Gonthier and Powers, J. Comput. Phys., 2000.
  • Powers, Phys. Fluids, 2004.
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SLIDE 5

Issues with Continuum Mixture Theories

  • Well-posedness not always straightforward.
  • Second law complicated.
  • Shock jumps not clearly defined for non-conservative

equations.

  • Consequent numerical difficulties.
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SLIDE 6

Inviscid Theory of Bdzil, et al.

  • First theory to unambiguously satisfy the second law.
  • Hyperbolic and well-posed for initial value problems.
  • Fundamentally non-conservative.
  • Some regularization needed for discontinuities.
  • No viscous cutoff mechanism for multidimensional

instabilities.

  • Grid-dependent numerical viscosity problematic.
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SLIDE 7

Viscous Extension

∂ ∂t (ρsφs) + ∇ · (ρsφsus) = C, ∂ ∂t (ρgφg) + ∇ · (ρgφgug) = −C, ∂ ∂t (ρsφsus) + ∇ ·

  • ρsφsusuT

s + φs (psI − τ s)

  • = M,

∂ ∂t (ρgφgug) + ∇ ·

  • ρgφguguT

g + φg (pgI − τ g)

  • = −M,
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SLIDE 8

Viscous Extension (cont.)

∂ ∂t

  • ρsφs
  • es + 1

2us · us

  • +∇ ·
  • ρsφsus
  • es + 1

2us · us

  • + φsus · (psI − τ s) + φsqs
  • = E,

∂ ∂t

  • ρgφg
  • eg + 1

2ug · ug

  • +∇ ·
  • ρgφgug
  • eg + 1

2ug · ug

  • + φgug · (pgI − τ g) + φgqg
  • = −E,

∂ρs ∂t + ∇ · (ρsus) = −ρsF φs , ∂ ∂t (ρsφsηs + ρgφgηg) +∇ · (ρsφsusηs + ρgφgugηg) ≥ −∇ · φsqs Ts + φgqg Tg

  • .
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SLIDE 9

Constitutive Equations

φg + φs = 1, ψs = ˆ ψs(ρs, Ts) + B(φs), ψg = ψg(ρg, Tg), ps = ρ2

s

∂ψs ∂ρs

  • Ts,φs

, pg = ρ2

g

∂ψg ∂ρg

  • Tg

, ηs = − ∂ψs ∂Ts

  • ρs,φs

, ηg = − ∂ψg ∂Tg

  • ρg

, βs = ρsφs ∂ψs ∂φs

  • ρs,Ts

, es = ψs + Tsηs, eg = ψg + Tgηg,

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SLIDE 10

Constitutive Equations (cont.)

τ s = 2µs (∇us)T + ∇us 2 − 1 3(∇ · us)I

  • ,

τ g = 2µs (∇ug)T + ∇ug 2 − 1 3(∇ · ug)I

  • ,

qs = −ks∇Ts, qg = −kg∇Tg, C = C(ρs, ρg, Ts, Tg, φs), M = pg∇φs − δ(us − ug) + 1 2(us + ug)C, E = H(Tg − Ts) − pgF + us · M +

  • es − us · us

2

  • C,

F = φsφg µc (ps − βs − pg).

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SLIDE 11

Equations of State Modified Tait equation for solid (correction courtesy

  • D. W. Schwendeman)

ψs(ρs, Ts, φs) = cvsTs

  • 1 − ln

Ts Ts0

  • + (γs − 1) ln

ρs ρs0

  • + 1

γs ρs0 ρs εs + q +(ps0 − pg0) (2 − φs0)2 ρs0φs0 ln

  • 1

1−φs0

  • ln

  2 − φs0 2 − φs (1 − φs)

1−φs 2−φs

(1 − φs0)

1−φs0 2−φs0

 

Virial equation for gas

ψg(ρg, Tg) = cvgTg

  • 1 − ln

Tg Tg0

  • + (γg − 1)
  • ln

ρg ρg0

  • + bg(ρg − ρg0)
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SLIDE 12

Viscous Dissipation Function

Φs = 2µs     ∇us + (∇us)T 2

  • strain rate

− 1 3(∇ · us)

  • mean strain rate

I    

  • deviatoric strain rate

:     ∇us + (∇us)T 2

  • strain rate

− 1 3(∇ · us)

  • mean strain rate

I    

  • deviatoric strain rate

.

  • similar expression for Φg.
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SLIDE 13

Dissipation: Clausius-Duhem Equation

I ≡ (−C) βs ρsTs + es − eg − pg(1/ρg − 1/ρs) Tg + ηg − ηs

  • +δ (us − ug) · (us − ug)

Tg +H(Tg − Ts)2 TgTs +φsφg µc (ps − βs − pg)2 Ts +φsΦs Ts + φgΦg Tg +ksφs∇Ts · ∇Ts T 2

s

+ kgφg∇Tg · ∇Tg T 2

g

≥ 0.

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SLIDE 14

Characteristics

  • Three real characteristics us, us, ug,
  • Three associated eigenvectors,
  • Not enough eigenvectors for eleven equations:

parabolic,

  • Eight additional conditions from boundary conditions
  • n Ts, Tg, us, ug.
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SLIDE 15

Numerical Method

  • One-Dimensional: Fortran 90 code

– Second order central spatial discretization – High order implicit integration in time with DLSODE

  • Two-Dimensional: FEMLAB software tool

– Finite element method for the form

∂q ∂t + ∇ · f(q) = s(q).

– Unstructured mesh

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SLIDE 16

1D Verification: Shock Tube

0.1 0.2 0.3 0.4 0.5 x (m) 300 305 T (K) 290 310 295

Tg Ts

0.001 0.01 0.1 ∆x (m) 0.01 0.1 1 L (K)

1

0.001 0.0001

slope=1.95 slope=0.75 A1 A2 inviscid analytical viscous numerical

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SLIDE 17

1D Verification: Piston-Driven Shock

0.1 0.2 0.3 0.4 0.5 x (m) 310 320 330 340 T (K) 300

solid gas B1

0.18 0.22 0.24 0.26 0.28 x (m) 305 310 315 320 325 T (K)

g

steady solution time-dependent solution

0.20

viscous shock in gas B3

0.37 0.38 0.39 x (m) 310 320 330 340 T (K)

steady solution time-dependent solution

0.36 300

s

viscous shock in solid B2

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SLIDE 18

1D Subsonic Piston-Driven Compaction

0.1 0.2 0.3 0.4 0.5 x (m) 0.5 1 5 10 50 p (MPa)

p

s

p

g

βs E1

0.1 0.2 0.3 0.4 0.5 x (m) 20 40 60 80 100 u (m/s)

u , u

s g

E3

0.1 0.2 0.3 0.4 0.5 x (m) 301 302 303 304 T (K)

T , T

s g

0.1 0.2 0.3 0.4 0.5 x (m) 0.2 0.4 0.6 0.8 1 φs

E2

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SLIDE 19

1D Dissipation: Subsonic Case

0.1 0.2 0.3 0.4 0.5 x (m) 50 100 150 200

I (MW/m /K)

3

Total Compaction Solid Momentum Diffusion

E

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SLIDE 20

FEMLAB vs. F90 Verification: 1D Shock Tube

x [m]

310

305 295

290

300

x [m]

1.4 x 10-3 0 0.1 0.2 0.3 0.4 0.5 0 0.1 0.2 0.3 0.4 0.5 R e l a t i v e E r r

  • r

T [K] g 0.5 1.0

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SLIDE 21

Narrow 2D Shock Tube vs. 1D Shock Tube

300 K 292 K 310 K 300 K x (m) 0 0.1 0.2 0.3 0.4 0.5

290 300 310 x (m) t = 50 µs

T (K)

g 0.0 0.1 0.2 0.3 0.4 0.5

2D 1D

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SLIDE 22

Small Energy Pulse: 2D Response

. . .

t = 18 μs t = 0 μs Solid Pressure small temperature perturbation radial pressure wave at ~ 2000 m/s reflection at wall

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SLIDE 23

Large Energy Pulse: 2D Response

φs

Max = 0.867 Min=0.730 (x,y) 0.040 0.000

  • 0.015

0 0.035 0.05 x (m) y (m)

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SLIDE 24

Conclusions

  • Diffusion enables use of simple numerical techniques.
  • Diffusion suppresses short wavelength instabilities,

e.g. Kelvin-Helmholtz.

  • Diffusion suppresses subgranular length scales.
  • Compaction dominates the dissipation.
  • Rigorous subscale physical justification for diffusion

models presently lacking.

  • Such justification necessary for a validated model.