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Numerical Simulation of
Granular Flow
Based on Micropolar Fluid Theory
Shin-Ichiro Serizawa/Tomoyuki Ito
(serizawa.shinichiro@gmail.com)
Needs of Granular Flow Analysis
 From Natural Phenomena to Industry
 Prediction of Natural Phenomena
 Landslide
 Avalanche
 Pyroclastic flow
 Industry
 Civil Engineering
 Agriculture
 Pharmacy
 Electrophtography
Numerical Analysis Method
 Distinct Element Method
 Each Particle Interactions are presented by Cundall Model
 Cundall, P.A., Strack, O.D.L., A Discrete Numerical Model for
Granular Assemblies, Geotechnique, 29-1(1979), 47-65.
 DEM Takes Huge Computing Cost.
Ct
Kt
Kn
Cn
m
rj
ri
mj
mi
Cundall Model
 Description of Granular Flow as the
Constitutive Law model is required.
 FEM/FDM and etc. can be applied to solve.
Reduction of Computational Cost
Hibler’s Rheology Model
 Numerical Model of the Sea Drift Ices
 Hibler, W. D., III. A Dynamic Thermodynamic Sea
Ice Model, Journal of Physical Oceanography, 9-4
(1979), 815-846.
 Viscosity coefficient h
 Decided by Principle Strain Speed
 If Large then Act as Plastic Flow
 Else if then Act as Viscous flow
 Mohr-Coulomb Yield Criterion
 Internal Friction Angle f  1 2 1 2 sin    f  
max
1 2
Psin
min ,
f
h h
 
 
  
 
Hibler’s Rheology Model
 Governing Equations
 Conservation Law
 Momentum
 Constitutive Equation
ij ij ij kk ij
1
P 2
2
  h   
 
    
 
i
ji,j
d
dt
   
v
f
k ,k
d
0
dt

 v
Problems of Hibler’s Rheology Model
 The Rotations of Particles are not Considered.
 The Grain Size is not Explicitly Described in
Constitutive Equation.
Micoropolar Fluid Theory
 Microstructure in Continuum
 Micro Rotation w
 Characteristic Length d
1
11
2
m32
m31
22
w3
d
12
21
3
v1
v2
Micoropolar Fluid Theory
 Governing Equations
 Conservation of Mass
 Momentum
 Angular Momentum
 Constitutive Equation
 Stress
 Coupled Stress
i
ji,j ijk jk i
d
I c
dt
 m     
w
i
ji,j i
d
dt
   
v
f
k ,k
d
0
dt

 v
 ij k,k ij i,j j,i c i,j  m h w  h w h w h w   
  j,i i,j
ij k ,k i
j,i i,j
kj r ijk
v v
2
v v
P v 2
22
h  w   h
    
  
 
 
     
   
Model Based on Micropolar Fluid Theory
 Kanatani, K., A Micropolar Continuum Theory
for the Flow of Granular Materials,
International Journal of Engineering Science,
17-4, (1979), 419–432.
 Mitarai, N. Hayakawa H. and Nakanishi, H.,
Collisional Granular Flow as a Micropolar Fluid,
Phys. Rev. Lett. 88, (2002), 174301.
Extended Hibler Model
 Viscosity
 Decided by Equivalent Strain Speed
 Micro Rotation Viscosity
 Angular Viscosity
 Pressure Equation
 Pressure is Non Negative value
max
Psin
min ,h

f
h
 
  
 
 
1
2
ij ij1 2 ij ji 2
ij3 ij
e e e e
d k k
2
g g
g
 
  
 
 
1
3
ij ij kk ije    
r f (d ) Const.h  
2
c
1
I
1
d
0
h h h 
max
0
0 0
0
0
P P










 
 

1
3
ij ij kk ijk    
Smoothed Particle Hydrodynamics
 Physics Quantities are expressed by Kernel
Function
 Lucy, L. B., A numerical approach to the testing of the fission
hydrodynamics, Astron., J., 82-12 (1977), 1013- 1024.
 Gingold R. A. Monaghan, J. J., Smoothed particle hydrodynamics:
Theory and application to non spherical stars, Mon. Not, Roy. Astron.
Soc., 181 (1977), 375-389.
Approximation by Kernel Functions
Example by SPH
 Schematic of Sand Pile Formation
0
0.1
0.2
0.3
0.4
0.5
0 0.25 0.5 0.75 1
Hieght(m)
x (m)
25 particles
50 particles
x
y
xmax
Result of Pseudo Viscous Fluid
 Broken Dam
MaxvMinv
0.0 4.91 (/s)-4.91
0.0 4.91 (/s)-4.91
Result of Extended Hibler Model
Velosity:v
Angular Velosity:w
Counter Clockwise
No Rotation
Clockwise
0.0 0.78 (m/s)
0.0 0.78 (m/s)
Velosity:v
Angular Velosity:w
Counter Clockwise
No Rotation
Clockwise
Parameters in Constitutive Equations
 Internal Friction Angle : f
 Characteristic Length : d
Internal Friction Angle
 Internal Friction Angle and Angle of Repose
0.0
0.1
0.2
0.3
0.4
0.5
0.0 0.2 0.4 0.6 0.8 1.0
70
60
45
30
15
y
x
15f  30f  45f  60f  75f 
Influence of Parameters in Equations
 Internal Friction Angle : f
 Characteristic Length : d
Characteristic Length and Fluidity
 Propagated Front Position
 as Index of Fluidity
0.8
0.9
0.9
1.0
1.0
1x10
-5
1x10
-4
1x10
-3
1x10
-2
1x10
-1
1x10
0
x
max
d
Hibler Model
Radius of Kernel Function:h
xmax
Conclusion
 The constitutive model of granular flow based
on micropolar fluid theory is presented.
 Part of granular matter flow with parallel and
rotational motion and the other part do not flow.
 The proposed model can reproduce sand pile unlike
fluid.
 Angle of repose depends on internal friction angle
of granular matter.
 The size of granular matter has an influence on
fluidity.
 The result is presented in The 63rd Japan
National Congress of Theoretical and
Applied Mechanics.
 Tokyo Institute of Technology
 2014.9.26

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Numerical simulation of Granular Flow Based on Micropolar Fluid Theory

  • 1. Numerical Simulation of Granular Flow Based on Micropolar Fluid Theory Shin-Ichiro Serizawa/Tomoyuki Ito (serizawa.shinichiro@gmail.com)
  • 2. Needs of Granular Flow Analysis  From Natural Phenomena to Industry  Prediction of Natural Phenomena  Landslide  Avalanche  Pyroclastic flow  Industry  Civil Engineering  Agriculture  Pharmacy  Electrophtography
  • 3. Numerical Analysis Method  Distinct Element Method  Each Particle Interactions are presented by Cundall Model  Cundall, P.A., Strack, O.D.L., A Discrete Numerical Model for Granular Assemblies, Geotechnique, 29-1(1979), 47-65.  DEM Takes Huge Computing Cost. Ct Kt Kn Cn m rj ri mj mi Cundall Model
  • 4.  Description of Granular Flow as the Constitutive Law model is required.  FEM/FDM and etc. can be applied to solve. Reduction of Computational Cost
  • 5. Hibler’s Rheology Model  Numerical Model of the Sea Drift Ices  Hibler, W. D., III. A Dynamic Thermodynamic Sea Ice Model, Journal of Physical Oceanography, 9-4 (1979), 815-846.  Viscosity coefficient h  Decided by Principle Strain Speed  If Large then Act as Plastic Flow  Else if then Act as Viscous flow  Mohr-Coulomb Yield Criterion  Internal Friction Angle f  1 2 1 2 sin    f   max 1 2 Psin min , f h h         
  • 6. Hibler’s Rheology Model  Governing Equations  Conservation Law  Momentum  Constitutive Equation ij ij ij kk ij 1 P 2 2   h             i ji,j d dt     v f k ,k d 0 dt   v
  • 7. Problems of Hibler’s Rheology Model  The Rotations of Particles are not Considered.  The Grain Size is not Explicitly Described in Constitutive Equation.
  • 8. Micoropolar Fluid Theory  Microstructure in Continuum  Micro Rotation w  Characteristic Length d 1 11 2 m32 m31 22 w3 d 12 21 3 v1 v2
  • 9. Micoropolar Fluid Theory  Governing Equations  Conservation of Mass  Momentum  Angular Momentum  Constitutive Equation  Stress  Coupled Stress i ji,j ijk jk i d I c dt  m      w i ji,j i d dt     v f k ,k d 0 dt   v  ij k,k ij i,j j,i c i,j  m h w  h w h w h w      j,i i,j ij k ,k i j,i i,j kj r ijk v v 2 v v P v 2 22 h  w   h                      
  • 10. Model Based on Micropolar Fluid Theory  Kanatani, K., A Micropolar Continuum Theory for the Flow of Granular Materials, International Journal of Engineering Science, 17-4, (1979), 419–432.  Mitarai, N. Hayakawa H. and Nakanishi, H., Collisional Granular Flow as a Micropolar Fluid, Phys. Rev. Lett. 88, (2002), 174301.
  • 11. Extended Hibler Model  Viscosity  Decided by Equivalent Strain Speed  Micro Rotation Viscosity  Angular Viscosity  Pressure Equation  Pressure is Non Negative value max Psin min ,h  f h          1 2 ij ij1 2 ij ji 2 ij3 ij e e e e d k k 2 g g g          1 3 ij ij kk ije     r f (d ) Const.h   2 c 1 I 1 d 0 h h h  max 0 0 0 0 0 P P                1 3 ij ij kk ijk    
  • 12. Smoothed Particle Hydrodynamics  Physics Quantities are expressed by Kernel Function  Lucy, L. B., A numerical approach to the testing of the fission hydrodynamics, Astron., J., 82-12 (1977), 1013- 1024.  Gingold R. A. Monaghan, J. J., Smoothed particle hydrodynamics: Theory and application to non spherical stars, Mon. Not, Roy. Astron. Soc., 181 (1977), 375-389. Approximation by Kernel Functions
  • 13. Example by SPH  Schematic of Sand Pile Formation 0 0.1 0.2 0.3 0.4 0.5 0 0.25 0.5 0.75 1 Hieght(m) x (m) 25 particles 50 particles x y xmax
  • 14. Result of Pseudo Viscous Fluid  Broken Dam MaxvMinv
  • 15. 0.0 4.91 (/s)-4.91 0.0 4.91 (/s)-4.91 Result of Extended Hibler Model Velosity:v Angular Velosity:w Counter Clockwise No Rotation Clockwise 0.0 0.78 (m/s) 0.0 0.78 (m/s) Velosity:v Angular Velosity:w Counter Clockwise No Rotation Clockwise
  • 16. Parameters in Constitutive Equations  Internal Friction Angle : f  Characteristic Length : d
  • 17. Internal Friction Angle  Internal Friction Angle and Angle of Repose 0.0 0.1 0.2 0.3 0.4 0.5 0.0 0.2 0.4 0.6 0.8 1.0 70 60 45 30 15 y x 15f  30f  45f  60f  75f 
  • 18. Influence of Parameters in Equations  Internal Friction Angle : f  Characteristic Length : d
  • 19. Characteristic Length and Fluidity  Propagated Front Position  as Index of Fluidity 0.8 0.9 0.9 1.0 1.0 1x10 -5 1x10 -4 1x10 -3 1x10 -2 1x10 -1 1x10 0 x max d Hibler Model Radius of Kernel Function:h xmax
  • 20. Conclusion  The constitutive model of granular flow based on micropolar fluid theory is presented.  Part of granular matter flow with parallel and rotational motion and the other part do not flow.  The proposed model can reproduce sand pile unlike fluid.  Angle of repose depends on internal friction angle of granular matter.  The size of granular matter has an influence on fluidity.
  • 21.  The result is presented in The 63rd Japan National Congress of Theoretical and Applied Mechanics.  Tokyo Institute of Technology  2014.9.26