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Different characteristics of the motion of a single particle on a bumpy inclined line

Gerald Ristow, François-Xavier Riguidel, Daniel Bideau

To cite this version:

Gerald Ristow, François-Xavier Riguidel, Daniel Bideau. Different characteristics of the motion of a

single particle on a bumpy inclined line. Journal de Physique I, EDP Sciences, 1994, 4 (8), pp.1161-

1172. �10.1051/jp1:1994246�. �jpa-00246976�

(2)

J. Phys. I £Fance 4

(1994)

1161-l172 AUGUST 1994, PAGE l161

Classification Pllysics Abstracts

64.60C 05.60 46.30

Dilllerent characteristics of the motion of

a

single particle

on a

bumpy inclined fine

Gerald H. Ristow

(*), François-Xavier Riguidel

and Daniel Bideau

Groupe Matière Condensée et Matériaux (**), Université de Rennes1, 35042 Rennes Cedex,

France

(Received

18 January1994, revised 24 Marcll 1994, accepted 15 April 1994)

Abstract. In order to better understand the rote of friction and disorder in segregation

mechanism in surface flow, we investigate the motion of a single bail of radius R on a one- dimensional bumpy fine made of balls of radius r. The smoothness is then controlled by

R/r,

the ratio of radii. In addition to experimental results for different ratios, we perform numerical simulations where the bumpiness disorder in spacing between the balls forming the fine is aise controlled. Different kinds of behavior are observed. In particular, we obtain

a regime where the bail quickly reaches

a constant mean velocity. In this regime, we investigate the friction forces during contacts and identify in a generalized model the regions which are dommated by solid friction or by loss due to collisions. We show that smaller balls get trapped more easily on a rough surface which might explain the origin of the segregation process found in rotating drums and sandpiles. We aise study this system for different values of the bumpiness of the fine and find conditions under which the constant velocity regime disappears completely.

1. Introduction.

Surface

phenomena

are of great importance in

rapid granular

flow but

despite

their wide use in industrial

applications

and expenments, a detailed

understanding

of the relevant parameters is not yet achieved. It was first studied

by Bagnold iii

who defined two flow

regimes (macroviscous

and

grain inertia)

in the case of a mixture of

grains

and fluid. The

grain

inertia

regime

in the

case of

high partiale

velocities is often described

by

a kinetic

theory (see

e-g- [2] but for denser systems or low

velocities,

the above theories have to be

greatly

modified to account for the

Coulomb-type

friction forces

along

surface contacts. This dualism of

granular

materials

(they

can behave like solids or like

fluids)

leads to instabilities which often have the form of

density

waves, observed in experiments [3] and numerical simulations

([4,

5])

(*) present address: Fachbereich Physik, Philipps-Universitàt Marburg, Renthof 6, 35032 Marburg, Germany.

(**) URA CNRS 804.

(3)

Dne of the most important mechanisms of

segregation

in

granular

media is surface flow [6].

When

partiales

of diiferent sizes move down an inclined bed or are part of an avalanche the

bigger

ones are found more

likely

on top at the end of the process. This

happens

aise m

a

rotating

drum or while

building

a

sandpile

where the

underlying partiales

net

being

part of an avalanche can be

regarded

as

being

fixed

(solid phase)

in a first approximation. If

two-dimensional

experiments

are

performed,

these

partides

form a one-dimensional

rough

fine where the scale of the

roughness depends

on the

grain

size distribution. This

roughness

aise

depends

on the size and the

shape

of the

rolling grains:

the

larger

the

grain,

the less stable its

equilibrium

when it is at rest, and the

longer

its mean free

path along

the

slope

when it flows.

Recent

experiments

in 2D drums and numerical simulations

using

diiferent models illustrate this

phenomenon

very well

iii.

In this context, we have

performed

experiments and numerical simulations ta get a better

understanding

of the individual behavior of a

single

bail

moving

down an inclined

bumpy

fine with controlled

roughness.

We define the smoothness as the ratio of the radius of the

single

bail

moving

down the fine ta the radius of the balls

forming

the fine

(RIT).

The motion is net easy ta understand and even for this

simple

case the energy balance between

gravity,

collision and friction forces leads ta

interesting

behavior

([8, 9]).

In a

previous

paper

[10],

we have

given

a

phase diagram showing

the diiferent

regimes

of

motion observed

experimentally

in a two-dimensional system. Here, we use the

hypothesis proposed by

Jan et al. [8] which was

developed

for the constant

velocity regime

and find that it can

only

be

applied

in a narrow range of the control parameter

RIT.

We then extend the

model

proposed by Jaeger

et al. [9] to describe the

general

behavior of the bail

moving

down and discuss the importance of the different forces as a function of the inclination

angle le),

the surface smoothness

(RIT)

and the

bumpiness

of the fine

le).

We present conditions under which the constant

velocity regime disappears completely

and for

particular

values of

angle

and size

ratio,

chaotic behavior can be reached, very similar to that obtained in the case of a

bouncing

bail

iii].

In the next section, we

explain

the experimental and numerical

techniques

we used. The results are

presented

and discussed in section 3.. In section 4., we present diiferent theoretical

approaches

to understand and

classify

our results and we conclude

by giving

an outlook on the

applicability

of our results to other

phenomena,

1-e- the

segregation

process.

2.

Experimental

and numerical system.

2.1 EXPERIMENTAL SETUP. Dur

experimental

setup is

slightly

dilferent from the one used in reference [8]: it is made up of a 2 m

long

mclined fine of 400 identical steel

spheres

of

diameter 5 mm. Each

sphere

is

touching

its

neighbors

and

they

are confined

by

a

L-shaped

flume sketched in

figure

1. The two sides X and Y can have a diiferent inclination

angle

ax

and ay with the horizontal. In ail our

experiments,

we have chosen ax

= 50° and ay

= 40°.

We then

study

the motion of a

single

steel

sphere

of variable size

moving

down

along

either

one of the two sides of the flume. In order to start the motion, we

give

it a small well defined initial

velocity.

2.2 NUMERICAL MODEL.

Concurrently

to these experiments, we have

performed

numerical

simulations on the motion of a bail on a

rough

inclined fine formed

by

balls

placed

in a disordered way. The distance between

neighbors

is

randomly

chosen between 2R and

2R(1+e),

where the disorder can be controlled

by

the parameter e

le

= 0 refers to the ordered case of

touching spheres).

A

snapshot

of the simulation for e

= o-à is shown in

figure

2. Periodic conditions are

imposed

to the fine so that the system can be considered as infinite.

(4)

N°8 MOTION OF A PARTICLE ON A BUMPY LINE 1163

x

y

Fig. 1. L-shaped flume used in the experiments with approximately 400 steel spheres.

~Î~

Ô

Fig. 2. ID motion of one bail on an inclined fine. Roughness of the hne is created by placing

balls randomly or net on it. In the random case, the distance between neighbours is randomly chosen between 2R

(touching spheres)

and

2R(1+ e).

The base of this simulation is the Molecular

Dynamics

method [12]. In

1979,

Cundall and Strack [13]

proposed

a model to describe the forces

acting

on

partiales

in an

assembly

of

spheres

on a

grain

size level which

they

called the distinct element method. Since then this

model has been extended and

slightly

modified to describe among others the mechanical

sorting

of

grains [14],

the shear-induced

phase

boundaries [15] the

origin

of convection cells [16] and the outflow from a

hopper ([17, 4]).

In Molecular

Dynamics simulation,

one solves Newton's equations of motion for each

particle

for successive times. The time axis is discrete and the order of the time step àt is crucial and has to be checked for numerical

stability.

Whenever two

particles

are doser than the sum of their

radii,

1-e-

they

have been

deformed, they

interact via normal and shear forces and the force on

partiale1,

caused

by partiale j

is given

by

Fij

" Fné+FSE

Fn = -kn

(ri

+ rj

(ri

rj

)é)~ inme~(éi

Fg

)é Il

Fs =

-isme~((éi fg )§

+ rioi +

rjoj

where

mimj

~~~

mi + mg

Here ri denotes the

position

vector of the ith

partiale,

il is the unit vector

pomting

from

partiale

to

j

and § is a unit vector

perpendicular

to

ilrotating

dockwise. The constant

kn

stands

for the

Young modulus,

in is the

damping

coefficient in the normal

direction,

is accounts for the transfer of translational energy into rotational energy and me~ denotes the effective

(reduced)

mass. For a

= 1, we are left with Hooke's law and for a

= 1-à we can

investigate

the Hertzian contact force due to

shghtly

deformable discs.

Normally,

the shear force Fs can

(5)

have two

regimes

where the transition is

given by

the friction coefficient ~t due to Coulomb's criterion which we

neglected

in our case (~t ~

cc)

since it introduces another parameter and it was found to

give

no

qualitative change

for the

investigated

setup.

We used cgs units

throughout

our simulations where the diarneter of the watt

partiales

was

1 cm. The

Young

modulus kn is lo~

gs~~cm~~~,

in

= 1000 Hz, i~

= 100 Hz and we used a

time step of àt = o-à x lo~~

s which assured numerical

stability.

The

relationship

between

our

damping

pararneter in and the

expenmentally

more

commonly

used restitution coefficient er can be calculated for Hooke's law

la

=

1) directly

from

equation Il) by comparing

the velocities

right

before and alter a collision. It is of the form

'In '~

~~~~(

[2)

1r + in

Ier)

For o

=

1-à,

one gets a very weak

velocity dependence

of in but

equation (2)

can still be used

as a

good approximation

over a wide

velocity

range which has been verified for our model

by

one of us

iii].

The chosen value of in in ail our simulations is

approximately equivalent

to a restitution coefficient of 0.7.

3.

Interpretation

of results.

3.1 PHASE DIAGRAMS. For a

general understanding

of the motion of the

single baÎÎ,

we

show m

figure

3 the

phase diagram

obtained in one dimension which is very similar to the

phase diagrams given

in

[loi

for one and two dimensions. As central parameters we used the smoothness

RIT

and the inclination

angle

8. In our expenments, we followed the motion of the

single

bail with a vider camera and calculated the

velocity

for diiferent

positions

on the fine. For our numerical

simulations,

we get the bail

velocity

every time step and monitor the

over 600 time steps

averaged

value. The phase boundanes for the diiferent bail motions

(which

will be

explained

in more detail in the next

paragraphs)

is

given.

We show the data from experiments and numerical simulations in the same

plot

for direct comparison.

For small inclination

angles

8 with the

horizontal,

the bail comes to a

complete

stop

(called regime A) regardless

of its initial

velocity.

The

gain

in

potential

energy, <

Ep

>m

2rmg sine,

is toc small

compared

to the

dissipation

due to friction or collisional fosses.

When the inclination

angle

is

increased,

one reaches a

regime

where the behavior of the bail

depends

on its initial

velocity.

For small values, the bail gets

trapped

in one of the next

valleys

formed

by

two balls. If the initial velocity is

high enough

to climb over at least the next bail,

one finds a regime of constant mean

velocity,

this

velocity being

defined at the top of each bail

forming

the fine

(called

regime

B) ([8, 9]).

The

phase boundary

for the case of a

high

initial

velocity

with the

regime

where the bail stops is shown in

figure

3 and for

RIT

= 1, we get an

angle

of

7°(exp.)

and

9.5°(sim.), respectively.

By

increasing the inclination

angle further,

we reach the regime where the bail starts to

jump,

1-e- the bail

rolling

down

might

not be in contact with any one of the balls

forming

the fine

(called regime

C). Such a situation is shown m

figure

2 and the

length

of the

jumps

seems to increase with time for small times. In this case, the

phase boundary

also

depends

on the initial

velocity

since a

triangular

lattice is stable up to an

angle

of 30°

(and

8 is less thon 30°

).

For a

high

initial

velocity

and for

RIT

= we get an

angle

of

20°(exp.)

and

17°(sim.).

On the base of numencal simulations, we found that this is

only

a transition

regime:

for very

long

times the

single

bail reaches a constant

velocity

which was two orders of

magnitude larger

than that obtained in

regime

B.

Unfortunately,

we do not see any chance to

verify

this

experimentally

smce fines

containing

a few thousand balls would be

required

and we will naine it the

regime

(6)

N°8 MOTION OF A PARTICLE ON A BUMPY LINE l165

experimental data

20 C numerical data

8

B

io

A

0

0.5 1.5 2 2 5

R/r

Fig. 3. Comparison of the phase diagram for the experiment

(thin hnes)

and the numerical simula- tion

(thick fines).

A: decelerated regime, B: constant velocity regime, C: accelerated regime

[umps).

of

increasing velocity (motivated by experimentally

accessible time behavior and to

distinguish

it from

regime B).

Figure

3 also shows that when the ratio

RIT

~ 0, the width of the constant

velocity regime

B decreases since the size of the

valley

between two balls becomes

bigger expressed

in bail diameters 2R of the bail

rolling

down. This means that the

trapping probability

increases for

RIT

~ 0. On the other

hand,

for

RIT

> 1 we found that the width of the constant

velocity regime

decreases when

RIT

increases.

The

experimental

points are connected

by

a thin fine and the numerical

points by

a thick fine to

guide

the eye. Both capture the essential features and for the

phase boundary

between

regimes

A and B the dilference is less thon 10$l for values of

RIT

> 1.2. In our numerical

simulations,

the

bump

in the upper curve for

RIT

= 1.2 is not

significant.

Since the type of motion for the

single

bail

depends strongly

on the initial

velocity

this

might

serve as an

indication for the

magnitude

of the numerical error.

Nevertheless,

we believe that an even better agreement con be achieved if more accurate values for the simulation parameters

kn,

in and is could be obtained from

experiments.

In our numerical

simulations,

we were able to

change

the

bumpiness

of the fine

by placing

the balls a random distance apart from each other. We used 70 balls with

periodic boundary

conditions and the distance between two of them was chosen from a uniform distribution

between 2R and

2R(1+ e).

We could therefore control the

bumpiness by

the parameter e

and e

= 0 reflects the ordered case discussed above. We find that the width of the constant

velocity regime

B also decreases when e increases. This is shown in

figure

4 where the dotted fine was obtained

by

a least square fit and for e > 0.2 we do not see this regime any more.

When e increases, the average hole size between balls gets

larger

and the

trapping probability

is increased for fixed

RIT.

This leads to the fact that for

high enough

values of e, we do not find a constant

velocity

regime before the bail gets

trapped.

This outlines the great influence of the disorder in this case.

(7)

B ,*

14 1

*

12

io

0.00 0.04 0 os 0 12 0 16 0 20

Fig. 4. Phase diagram for our numerical simulations for varying disorder of the fine. The dotted fines are a least square fit and show that for

a finite disorder ec Cz 0.2 the constant velocity regime B

disappears completely.

3.2 CONSTANT vELociTIEs IN REGIME B. As a first

comparison,

we have

performed

ex-

periments comparable

to those of reference [8] but we used up to 400 balls. Moreover the radius of the balls

forming

the fine

(r)

and the radius of the

single

bail

rolling

down

(R)

was

not

necessarily

the sonne. We

investigated

the average

velocity

of the

single

bail in the constant

velocity regime

B for diiferent values of the inclination

angle

8. The measured results for four diiferent values of

RIT

are shown in

figure

5. The

change

in

slope

of a curve for a

given

value of

RIT

for

higher

velocities indicates the

beginning

of the next

regime

C where the

partiale

starts to

jump.

This transition seems to be smoother for smaller values of

RIT, making

the

detection of the

phase

boundaries more difficult. It is also visible in

figure

7 at the end of the measured curves. One also notes in

figure

5 that the

slope

of a curve for a fixed value of

RIT

becomes steeper when the

angle

decreases.

In

figure

6, we show the data obtained

by

our numencal simulations for the same values of

RIT

and the parameters in = 1000, i~ = 100 and a

= 1.5

Ii.e. using

a Hertzian contact

force).

The

position

of the curve can be fine tuned

by adjusting

the parameters kn, in and i~. The data we present in this and the next section use values of the

right

order of

magnitude

since

exact values of the collision laws are hard to get

experimentally. However,

m our numerical

model we

neglected

the

slight dependence

of kn on the mass of trie

partiale. Keeping

m mind that

by using

real

physical

units m our numerical simulations we do not have a free parameter

to

adjust

our

length

and time scales the agreement between

figures

5 and 6 is remarkable. The

starting point

in sine of each curve agrees within 15-20$l close to

RIT

= and the diiference

m the initial

velocity

is less than 15$l for ail curves. For

higher

constant velocities vm, trie differences become

bigger

but we believe that more accurate values for kn, in and i~ and the

right dependence

of kn on the mass of the balls will lead to an even better agreement. One should also note that due to our

expenmental

setup, where the bail is forced to roll on one side of the

I<shaped

flume

(see Fig. l).

This constant

rubbing

leads to an additional friction force not considered in our numencal simulations. We tried to determine the influence of this

(8)

N°8 MOTION OF A PARTICLE ON A BUMPY LINE 1167

20

R/r=0.S - R/r=1.0 +- 16 R/r=1.6 é- R/r=2.0 -

12

Vm

s

4

0

0 o-1 0.2 0.3 0.4

s1n8

Fig. 5. Variation of vm in

cm/s

as a function of sine for our expenments for different values of

R/r.

30

R/r=0 8 -

R/r=1.0 +-

R/r=1.6 é- R/r=2.0 -

20

Vm

io

0

0 01 0 2 0 3 0 4

sin 8

Fig. 6. Same as figure 5 but now for our numerical simulations with ~tn

= 1000 and ~ts

= 100.

additional friction

by

varymg the inclination

angles

ox and ay.

Unfortunately,

this could

only

be done m a very narrow range to avoid that the bail would

jump

over the borders in

regime

C and does not lead to diiferent results. We also

thought

about using a

U-shaped

flume similar to that in reference [8] but the additional collisions with the two vertical watts seem to

be even worse. We feel that our model with better

adjusted

parameters can even be used for

quantitative

companson with

expenmental

data and believe that the contact forces are well described

by

the

proposed

model.

(9)

4. Characterization of trie

general

motion.

4.1 MODEL oF JAN ET AL.. In a recent

experiment,

Jan et al. [8] studied the motion of a

single

bail on an ordered fine

le

=

0)

made of balls of the same kind for three types of balls and

a fixed

roughness (RIT

=

1). They

found the three

regimes

described above and

proposed

a

theoretical

description

for the constant

velocity regime

B to find the

velocity

vm as a function of the

experimental

pararneters. The

velocity

vm was obtained

by writing

the balance between the

potential

energy diiference and the energy lost in inelastic collisions and

by

friction on the

plane, along

an

elementary path

ôx

= 2T defined as the distance between two successive

collisions,

or between two

neighboring

balls [8]:

mg2T

sin 8

=

kmv$

+

~tmg2T

cos 8

,

(3)

where m stands for the mass of the

bail,

g the acceleration of

gravity,

k is the collision coefficient

(related

to coefficient of

restitution),

and ~t a friction coefficient. This equation leads to a constant

velocity

of the form

vm =

)~ (sin

8 ~t cos

8) (4)

By dividing

the

right

hand side

by

the left hand side in

equation (3)

one is left with

g211Ù8

~

~~°~~~

~~~

The first term on the

right-hand

side measures the collision part and the second term the friction ratio of the energy

dissipation.

Using

their

experimental

determination of the diiferent parameters in

equation là),

the authors found that each of these parts are

roughly equivalent,

the friction part

being larger

at small

angles,

the collision part at

large angles.

If we want to compare these results with our

experiments

or numerical

simulations,

we have to take into account three facts

. the friction is a

priori

more considerable in the above descnbed

experimental

setup due to the two walls of the flume

. the size of the system is infinite in our numencal simulations, and of the order of 400

sphere

diameters

(compared

to 220 in Ref. [8]) in our

experiments

. our

numencally

studied systems can be disoTdeTed

The above fine of

thoughts, equations (3)-(5),

is also valid for

RIT #

1 but R does not enter the formulae. We therefore expect that

they

are

only

valid close to

RIT

= 1 and tested this

ansatz for the

velocity

vm obtained in our experiments and numencal simulations. We found

that it

only

worked well in the range <

RIT

< 2. For smaller values of

RIT,

the theoretical

curve did not capture the

sharp

increase in the

slope

when

decreasing

the inclination

angle

8.

Also for values of

RIT

greater than 2 the

predicted slope

was too steep.

Since we are interested in a

general description

which captures all of the observed phenomena,

we have to extend the above model.

4.2 MODEL oF JAEGER ET AL.. In 1990,

Jaeger

et ai. [9]

investigated

the forces

acting

on

a

single grain moving

on a surface made

by

other

grains.

No

assumption

about the

underlying

surface was made and the

general

form of the forces

acting

on the grain is

mù=a-F, (6)

(10)

N°8 MOTION OF A PARTICLE ON A BUMPY LINE l169

where m and v stand for the mass and the

velocity

of the

grain.

On the

flght

hand

side,

the first term a stands for the

driving force, usually gravity,

and the second term is a

general

friction force which accounts for ail forces

during grain-grain

contacts. The latter is of the form

~

l

/flV~ ~'~~~

' ~~~

where a,

fl,i

are material

dependent

parameters. For

high velocities,

we are left with F c~

v~ which was

already

studied

by Bagnold iii

and for low velocities one reaches trie solid friction

regime. By adjusting

the three parameters, one con

smoothly interpolate

between

these

regimes.

If

~~

> l,

equation Ii)

has a minimum at vo "

~~ l)Ifl

and one gets

'f 'f

an unstable

region

for velocities 0 < v < vo This is the situation we observe in our

experiments

and numerical simulations. There are two stable solutions for the

velocity

vm and the final state

depends

on the initial

velocity

of trie bail.

4.3 GENERALIzED MODEL. In our case, the

driving

force is

given by

a = mg sin8 and

we are

looking

at the constant

velocity regime

where ù

= 0. If we consider the ordered case

le

=

0),

we can write a

generalized

form of

equation (6) by looking

at the losses due to collisions and friction:

àp

a = mg sin 8

= F

=

j

àp

AN

"

W $

AN Al

"

~?~ S

àt '

j8)

where N stands for the number of

collisions,

for the travelled distance and

àpi

is the

averaged

loss between two collisions

(àp

for AN

collisions).

One sees

immediately

that

allât

= v and

in our case for the ordered line

àNlàl

is constant since we have one collision on each bail

forming

the fine in the stable

regime

B

(which

was checked

by

numencal

simulations).

Thus the

only

variable which

might depend

on the

driving

force is

àpi.

The

problem

is more

complex

in two dimensions: the term

àNlàl

may

depend

on

8,

the inclination

angle,

and also on the smoothness

RIT.

We have found in 2D

[loi

that the friction coefficient <

f

> = < F

>Im

c~

(RIT)~~.~

but we were unable to

explain

the exponent of -1.5

theoretically.

Is it connected with the

specific

contact laws

during collisions,

to the

disorder,

etc.?

In

figure

7, we show

àpi

as a function of the constant

velocity

vm for two different ratios

RIT.

The

general

behavior is as

expected

and for

RIT

= 1-fi, one sees

clearly

the

beginmng

of the regime which is

proportional

to v

giving

a force F c~ v~ since the loss due to friction is

negligible.

The

change

m

slope

at the end of the curves is due to the

beginning

of

regime

C.

In

figure

8, we show the same quantities as above but for our numerical simulations using four values of the

roughness RIT.

For small velocities, we could

verify by

a

log-log plot

that

àpi

scales like

1Iv

and thus leads to a behavior

resembling

solid friction in the limit v ~ 0.

This is

only

due to the geometry of the

problem

since we do not account for static friction in

our force laws

(Eq. Il )).

For

high velocity,

the same

procedure

reveals a

regime proportional

to

v which is visible m the

plots

for

RIT

= 1.6 and

RIT

= 2.0. For certain parameter ranges

le-g- RIT

= 1-o in our numerical

simulations),

one finds a wide region where

àp,

is

nearly

constant

which leads to a

general

friction force of F c~ v. This is the law we found in our expenments on a two-dimensional inclined

plane

with controlled

roughness ([10, 18])

and we also showed that the friction force varies as

(RIT)~~

~ This law could not be derived from the geometry of the

JOURNAL DE PHYSIQUE T 4 N'8 AUGUST 19Q4 42

(11)

0.030

R/r=10 +- R/r=1.6 é-

0 029

0 015

0.028

AP> APT

0.027

0.013 0 026

0.025

4 S 12 14 4 8 12

vm vm

Fig. 7. Averaged loss Ap~

lin

arbitrary

units)

between two collisions

(experiments).

0 042 0 028

R/r=0 8 - R/r=1.0 +-

0.038

0.024 0.034

àp~ àp~

0.030

0.020

0.026

0.022 0.016

5 15 25 5 15 25

vm vm

0.015 0.014

R/r=1.6 é- R/r=2.0 -

0.013 Ô.ol?

APT APT

o.oit o,oie

0.009 0.008

5 15 25 5 15 25

vm vm

Fig. 8. Same as figure 7 but for data obtained by numerical simulations.

(12)

N°8 MOTION OF A PARTICLE ON A BUMPY LINE l171

problem

and we believe that the contact forces

during partiale

collisions are

responsible

for it.

To test this

hypothesis,

we

investigated

with our numerical simulations the average loss

àpi

as a function of the

velocity

vm

(see Figs.

7 and

8)

for diiferent values of the surface

roughness

in the

region RIT

E

[0.8,

2]. The

procedure

goes as follows: we

plot

ail four parts of

figure

8

on one

graph

and read off the values of

àpj

for a

given

vm for the various ratios

RIT.

We then make a

log-log plot

of

àp,

as a function of

RIT by averaging

over different values of vm and

obtain for a Hertzian contact force

la

=

1.5)

a

scaling

of

àpi

c~

(R/T)~~.~~°.~, regardless

of the parameters in and is. For Hooke's law

la

=

1),

we obtain

àpi

c~

(R/T)~~.°".~

which is

significantly

different. Therefore we condude that the friction law

proportional

to

(R/T)~~.~

found in

experiments

and numerical simulations is

essentially

caused

by

the exact form of the contact forces

during

collisions in one and two dimensions.

The

proposed writing

of the

generalized

friction force in

equation (8)

has the

advantage

that

it can

easily

be extended to the disordered case

le

>

o)

or to two dimensions. The

only quantity

one has to measure or estimate is AN

/àl

to obtain the

averaged

loss of momentum between

two successive collisions which can then be

compared

with the one-dimensional ordered case studied above.

5. Conclusions.

We

investigated by

means of

experiments

and numerical simulations the movement of a

single

ball on a one-dimensional line with controlled

roughness

and

possible

disorder in the arrange- ment of the balls

forming

the line. We extended the

phase diagram

given in

(loi

and found that in the disordered case, the constant

velocity regime disappears

for e > ec Cz 0.2. In a

generalized model,

we could

give

an

expression

for the average loss

àpi

between two collisions which is valid in the ordered as well as in the disordered case and in any dimension. We found

àpi

c~

(R/T)~~.~

and the exponent

depends

on the contact forces

during

collisions.

Concerning

the

trapping

and

segregation

mechanism on the surface of avalanches in two

dimensions,

it is clear from our

investigations

on this

simple

model that smaller

grains

have

a shorter mean free

path

in an avalanche and therefore get

trapped

in the middle

region

of

a

rotating

drum in the

long

run. From the

phase diagram

in

figure

3, one sees that the stable

region

of no motion extends to

higher

values of 8 for smaller

grains.

This is even more

pronounced

if a disordered surface is considered

(see Fig. 4).

The reason is seen in

figure

8 where the motion in the constant

velocity regime

is very close to the static friction limit for smaller ratios of

RIT (Figs. la)

and

16)) leading

to a

scaling

of

àpi

c~

llv,

as

opposed

to

figures (c)

and

Id).

Acknowledgments.

We would like to thank our

colleagues

of the GMCM and

especially

Alex Hansen for very inter-

esting

discussions about this work. We also

acknowledge

support from the ATP CNRS Matéri-

a~~

Hétérogènes

from the

Groupement

de Recherches CNRS

Physiq~e

des Milie~~

Hétérogènes Compie~es.

References

Ill

Bagnold R-A-, Froc. R. Soc. London A 225

(1954)

49.

[2] Jenkins J-T- and Savage S-B-, J. Fluid Mech. 130

(1983)

186;

Lun C.K.K., Savage S-B-, Jeffrey D.J. and Chepumiy N., J. Fluid Mech. 140

(1984)

223.

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[3] Baxter G-W-, Behringer R-P-, Fagert T. and Johnson G-A-, Phys. Rev. Lent. 62

(1989)

2825;

Drake T.G., J. Geophys. Res. 95

(1990)

8681.

[4] Ristow G-H- and Herrmann H-J-, Density Patterns in Granular Media, HLM preprint 1993.

[Si Pôschel T., J. Phys. I £Fonce 4

(1994)

499;

Lee J., Phys. Rev. E 49

(1994)

281.

[fil Jullien R. and Meakin P., Nature 344

(1990)

425-427;

Williams J-C-, Ghem. Process. Suppl.

(1965);

Savage

S., Interparticle percolation and segregation in

granular

materials, Developments in En- gineering Mechanics, A.P.S. Selvadurai Ed.

(Elsevier

Science Pub. B-V- Amsterdam, 1987) [7] Ristow G-H-, Cantelaube-Lebec F. and Bideau D., Avalanches

in a two-dimensional rotating drum: experiment and simulation, preprint 1994;

Clément E., Duran J. and Rajchenbach J., Mélangeage d'un Matériau Granulaire dans un Tam- bour rotatif, Congrès de Mécanique, Lille

(sept.

1993);

Baumann G., Jobs E. and Wolf D.E., Fractals 1

(1993)

767.

[8] Jan C.D., Shen H-W-, Ling C.H. and Chen C.I., Proc of the Ninth Conf of Eng. Mech

(1992)

pp. 768-771.

[9] Jaeger H-M-, Liu C.-H., Nagel S-R- and Witten T.A., Europhys. Lent. Il

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619.

[loi

Riguidel F-X-, Jullien R., Ristow G., Hansen A. and Bideau D., J. Phys. I France 4

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261.

Ill]

Tullifaro N-B- and Albano A.M., Am. J. Phys. 54

(1986)

939;

Duran J., Europhys. Lent. 17

(1992)

679.

[12] Allen M.P. and Tildesley D.J., Computer Simulations of Liquids

(Clarendon

Press, Oxford, 1987) [13] Cundall P. and Strack O.D.L.,

Géotechnique

29

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47.

[14] Haff P.K. and Werner B-T-, Powder Technol. 48

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239.

[15] Thompson P-A- and Grest G-S-, Phys. Rev. Lent. 67

(1991)

1751.

[16] Taguchi Y.-h., Phys. Re~. Lent. 69

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1367;

Gaffas J-A-C-, Herrmann H-J- and Sokolowski S., Phys. Rev. Lent. 69

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1371.

[17] Ristow G-H-, J. Phys. I France 2

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649; Int. J. Mod. Phys. G 3

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