Computer Simulation of Granular Matter: A Study of An Industrial Grinding Mill By John Drozd.

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Computer Simulation of Granular Matter: A Study of An Industrial Grinding Mill By John Drozd

Transcript of Computer Simulation of Granular Matter: A Study of An Industrial Grinding Mill By John Drozd.

Page 1: Computer Simulation of Granular Matter: A Study of An Industrial Grinding Mill By John Drozd.

Computer Simulation of Granular Matter:

A Study of An Industrial Grinding Mill

By John Drozd

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Outline• Introduction and motivation.

• Event driven algorithm and formulae.

• Crushing forces.

• Discussion and analysis– Verification– Parameters– Steady state– Mean square displacement– Circulation

• Conclusions and recommendations.

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Granular Matter• Granular matter definition

– Small discrete particles vs. continuum

• Granular matter interest

– Biology, engineering, geology,

material science, physics.

– Mathematics and computer science.

• Granular motion

– Energy input and dissipation.

• Granular experiments

– Vibration

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Small AmplitudeSurface Waves

3-Node Arching

Large AmplitudeSurface Waves

C. Wassgren et al. 1996

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Other Phenomena in Granular Materials

• Shear flow

• Vertical shaking

• Horizontal shaking

• Conical hopper

• Rotating drum

• Cylindrical pan

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Cylindrical Pan Oscillations

Oleh Baran et al. 2001

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HarrySwinneyet al. 1997

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Harry Swinney et al. 1997

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Raw Feed

Grinding Media, Rods

VibratorMotor

GroundProduct

Vibratory Drum Grinder

IsolationSpring

Reactor Springs

Vibratory Drum Grinder

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Goal

• Find optimum oscillation that results in a force between the rods which achieves the ultimate stress of a particular medium that is to be crushed between the rods.

• Minimize the total energy required to grind the medium.

• Mixing is also important.

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Typical Simulation

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Event-driven Simulation Without Gravity

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Event-driven Simulation With Gravity

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Lubachevsky Algorithm

• Time values – Sum collision times

• Heap data structure– Disk with smallest time value kept at top

• Sectoring– Time complexity O (log n) vs O (n)– Buffer zones

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Rod 1 collides with Rod 2 with a collision time = 58

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Rod 2 collides with Rod 3 with a collision time = 124

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Rod-Rod Collisions

• Treat as smooth disk collisions

• Calculate Newtonian trajectories

• Calculate contact times

• Adjust velocities

02 2222 ijijijijij rtbtv

||2/ ijijijji vrbvv

ijijij vrb

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A Smooth Disk Collision

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Coefficient of Restitution• e is calculated as a velocity-dependent restitution

coefficient to reduce overlap occurrences as justified by experiments and defined below

• Here vn is the component of relative velocity along the line joining the disk centers, B = (1)v0

, = 0.7, v0=g and varying between 0 and 1 is a tunable parameter for the simulation.

0

0

,

,1

vv

vvvBve

n

nnn

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Rod-Container Collisions

22

22

2

1rRytgtvytvx yx

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Typical Simulation

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Circulation• The net circulation of the whole system was

calculated by first calculating the angular velocity of the vortex about the center of mass of the system and then using the formula

• where is the angular velocity of rotation or vorticity of the system and rmax is the distance from the farthest disk to the center of mass of the system.

2max22 rdAdA

2 V

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Circulation• The angular velocity of the vortex was calculated using the

formula

ii

ii

akvvaN

ˆˆ11

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Typical Time Averaged Velocity Field

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Net Circulation () vs Time (t)

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Measuring Disk Disk Forces as Collision Energies

• For a disk-disk collision, the collision energy can be calculated as

• where , and is the relative normal velocity between the disks before a collision.

2,2

1relneffc vmE

diskeff mm2

1 relnv ,

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Measuring Disk Container Forces as Collision Energies

• For a disk-container collision, the collision energy can be calculated as

• where and is the dot product of the velocity of the disk before the collision and a unit vector of the container surface normal , that is calculated as

2,2

1relneffc vmE

diskeff mm relnv ,

22,yx

tdyd

vyxv

vyx

reln

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Measuring Forces as Collision Energies

• These collision energies can be compared to the modulus of toughness of the material that is to be crushed between the disks.

• The modulus of toughness is defined as a strain-energy density, u, taken to the strain at rupture R using the formula

R

o xx du

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Parameters for Simulation

• The program was run using the parameters (g, , , y, Ay, e0, eW) and a simulation that produced a realistic motion was selected (y=126 rad/s= 20 Hz, Ay=1.5 cm, e0=0.4, eW=1.0).

• By a realistic motion, we mean that the disks would cluster together at the bottom of the container within a relatively short period of time with few overlaps.

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Total Kinetic Energy (KE/M) vs Time (t)

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Power Spectrum of Total Kinetic Energy ( P() )

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Mean Square Displacement Plots: Mixing Times

• Fixed time origin t0 formula:

• Moving time origin t‘ formula:

N

iiitt

tytrtytrN

r1

002 1

0

t

N

iii

ttt

tytrtytrNN

r1

'

2 ''11

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Mean Square Displacement (< r2 >) versus time (t)

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Phase Diagram: Amplitude (A) vs Frequency (y)

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Time Averaged Net Circulation () vs Frequency (y)

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Non-dimensional Parameter (/(Ay2 y)) vs Frequency (y)

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Circulation at Sloped Part of Curve

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Circulation at Leveling Off Part of Curve

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Velocity Field Snapshot for Typical Simulation

Axis of Symmetry

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0, 2

/ 2

3/2

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Number of Different Disks that Experience Mean Collision Energy (ni) i times vs Time (t)

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Conclusion

By quantifying the crushing forces in terms of collision energies and studying circulation and mixing, this thesis has outlined a thorough systematic approach to studying the grinding mill industrial crushing problem.

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Next Steps• Finer test matrices and calibrating results with

experiments• Compare the percentages of the medium that was

crushed and compare to the n1, n2, … and saturation times for various simulations using different amplitudes and frequencies of oscillation.

• Determine the frequency and amplitude for an optimum oscillation, that is, to minimize the energy required to get a well-mixed container with all the rods experiencing the mean (threshold) collision energy. This is the solution to the task outlined in this thesis.

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Recommendations for Future Work

• Incorporating horizontal container oscillations.• Incorporating rod rotations.• Using a mixture of different sized rods.• Using different quantities of rods and different

container sizes.• Study situations with different rod-wall boundary

conditions: multiple vortices.• Parallelization and sectoring using many numbers

of rods.

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Acknowledgements

• Brad Smith and Kirk Bevan

• Dr. Oleh Baran

• Dr. Ivan Saika-Voivod

• Dr. Sreeram Valluri

• Drs. Peter Poole and Robert Martinuzzi

• NSERC