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HAL Id: jpa-00246903

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Submitted on 1 Jan 1994

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Behaviour of a sphere on a rough inclined plane

François-Xavier Riguidel, Remi Jullien, Gerald Ristow, Alex Hansen, Daniel Bideau

To cite this version:

François-Xavier Riguidel, Remi Jullien, Gerald Ristow, Alex Hansen, Daniel Bideau. Behaviour of a sphere on a rough inclined plane. Journal de Physique I, EDP Sciences, 1994, 4 (2), pp.261-272.

�10.1051/jp1:1994106�. �jpa-00246903�

(2)

Classification

Physics

AbstJ.acts

46.30 64.60 68.22

Behaviour of

a

sphere

on a

rough inclined plane

François-Xavier Riguidel (~),

Remi Jullien

(2),

Gerald H. Ristow

(1),

Alex Hansen

(')

and Daniel Bideau

(1)

(') Groupe

Matière Condensée et Matériaux

(*),

Université de Rennes I,

Campus

de Beaulieu, 35042 Rennes Cedex, France

(2) Laboratoire des Sciences des Matériaux Vitreux (~*). Université de Montpellier II, Case 069, Place

Eugène

Bataillon, 34095 Montpellier Cedex 5, France

(Received ii Jane J993, revised 7 September J993,

accepted

J2 October J993)

Abstract. The tlifferent states of a bail on a rough indmed plane are analyzed from

experimental

results and numencal simulations. The conditions of static

equilibrium

are given. The control parameters are the inclination angle of the plane antl the surface roughness. Then, we propose a

«phase

tliagram

» for the motion of the bail. These results are expectetl to be useful m

untlerstantling

the

ongin

of the

segregatîon

effects on the surface of a

sandpile.

This paper is devoted to the

study

of the different regimes goveming the motion of one

particle

on an indmed surface of controlled

roughness (or smoothness).

The

goal

of this work

is to reach a better

understanding

of various

phenomena

occurrmg at the surface of a

flowing granular

medium,

especially segregation

:

generally

if one observes the surface of a

granular

medium

(e.g,

a sand

pile),

the

Iarger grains

are at the lower part, while the smaller

grains

are at the top.

Une of the most

important

mechanisms of

segregatîon

is the surface flow

il -3]

: the grains

near the surface move on a

rough

surface which is the

loyer below,

and the

roughness

seen

by

a

grain depends

on its own size

compared

to the size of

bumps

beneath it. The

forger

the

grain,

the less stable its

equilibrium position

when not

moving,

and the

longer

its « mean free

path

»

L

along

the

slope

when moving. This

explains why

one

always

finds the

Iargest grains

at the bottom of

piles. Experiments

using a two-dimensional drum

[4]

confirrn that surface flow is an important mechanism of

segregation.

The

equilibrium

of a

sandpile

is

generally

defined from the

angle of

repose 0~, which is the

slope

of a

pile

built

dynamically [5, 6]. However, starting

from this

angle,

such as in

experiments

on

avalanches,

one can define the maximum

angle ofstability 0~ [5] (or angle of

(~) URA CNRS n 804.

(.~*) URA CNRS n° II19.

JOLRNAL D~ PHYSIQUE T 4, N' 2 FEBRUARY <994

(3)

niaJ.gmctl stability [6])

as the maximum

angle

for which the

pile

is Table. For

examp[e,

this

angle

may be measured

by tilting

the

pile

until an avalanche occurs.

However,

according

to the initial conditions and the

angle

o between the inclined

plane

and the horizontal, the motion and the

equilibrium

of a

particle

on a

rough

inclined surface i~ not a

simple problem

to describe

[7, 8].

Dur

simplified

model pennits a formai and

relati~ely complete investigation

of this

problem (roughness

and inclination

angle

are both control

parameters),

even if a direct

analogy

with the surface of the

sandpile

is non very strong. If one i~

only

concemed

by

the static behaviour, 1-e-

by studying

the motion of the bail without any initial energy, we can define a

stability

threshold 0~. For ~

o,,

the hall is stable,

trapped

in a

well at the surface.

Agam

with respect to

equihbrium

of

piles, 0,

is a

locally

defined

angle

of

maximum

stability, depending mamly

on the geometry of the grains and that of the ~y;tem and

to a fesser

degree

on the friction coefficient.

If one gwes an initial kinetic energy to the hall, the

problem

becomes different. The hall

moves on the surface m a sort of directed random walk.

Starting

with an initial energy, the

motion is first decelerated and, for small

enough

H, it stops. For

larger

value~ of 0, the hall reache~ a constant

speed,

such as m the sedimentation of one

partide

submitted to Stokes

drag

force. When the

angle

increases above a threshold value

(,

the hall

jumps

on the

plane,

and the scale of the motion is

completely changed.

This

regime

seems to be a transient one : the numefical simulations show thon after a very

long

lime, a new stationary regime i~ reached,

with a constant

speed

and small

jumps.

The paper is

orgamzed

in the

following

manner in the first section we pre~ent the resu[t~ of the

experimenta[

and the numencal methods we used in this

study.

The second ~ection

describes our results concerning static behaviour, whereas we present in section three a

<~

phase diagram

» conceming the different kinds of behaviour observed in the

dynarnic

ca~e.

1.

Experimental

and numencal system.

We want to model the surface of a «

sandpile

)>, but with control parameters which are the

slope

of the

pile,

and the

roughness

of it~ surface. In order to do this, we use an inc[ined

glas~

plane

P (one meter

long,

70 cm wide, and cm

thick),

which can have a variable

angle

i&.ith the horizontal. The

roughness

of the

plane

is obtained

by ~ticking

smooth

glas~ spheres

(of radius 0.1 1) on contact paper fixed on the

plane. Figure

shows a part of a

rough

~urface

Fig.

l Photograph of a pan of a rough surface obtainetl by sticking gla,~ beatl~ (tliametei 0.5 mm on

a

plane.

The obtainetl

packmg

fraction is C 0.7.

(4)

obtained

by

this method. The two-dimensional

(2D) packing

is

homogeneous,

with a

packing

fraction C 0.70-0.75. This is far from the usual

packing

fraction for dense disordered 2D

systems (C 0.82) [9],

but seems to

give

a

roughness comparable

to that observed at the surface of a

pile.

Note that this 2D

packing

is a disordered one. The radius of the

spheres moving

down the

plane

P is

R,

and we define here the smoothness 4l of the

plane

as the ratio Rli

(the roughness

in this

particular

case

being

the ratio

ilR).

In one-dimensional

ID)

numerical

simulations,

we build an indmed row of

equal spheres,

whose distance between

neighbours

con be

randomly

fixed between 2 r

(touching spheres)

and

2>.(1+ e):

see

figure

2. This mimics the disorder observed in 2D

experiments

and simulations. The motion of one ball on this inclined row is studied

by

using molecular

dynamics

simulations

developed by

one of us

[loi.

The hall can rotate and we consider

dissipation

and

dynamic

friction

during

collisions. As an

integration scheme,

we use a third- order

predictor-corrector algorithm [1Il.

Periodic

boundary

conditions are

imposed,

in such a way that

long

distance motion con be studied.

8

Fig. 2. ID motion of one ball on an inclined line. The roughness of the litre is createtl by placing balls

at rantlom or equally tlistanced positions. In the rantlom case, the distance between neighbours is

randomly

chosen between 2 r

(touching

spheres) and 4 r.

From the 2D numerical

point

of view, the ensemble of

equal

sized small

spheres

stuck on the

plane

P is modeled

using

the random

sequential adsorption

model m two dimensions

(RSA) just

below its

jamming

threshold, which is at a

packing

fraction of C~ = 0,547

[12].

In

figure

3 we show an

example

of such a

configuration,

with a

packing

fraction of

C

=

0.52,

built on a square of

edge length

L

=

180 1, where r is the radius of the small

sphere,

with

periodic boundary

conditions at the

edges

of the square. The

geometrical properties

of such RSA

packing

near the

jamming

threshold have been

extensively

studied in the past

[12].

We have

only reproduced

here the

computations

that are necessary for the purpose of our

study.

We simulate the motion of a

larger sphere by

assuming that it

always

stays in contact with at least two smaller

spheres dunng

its entire

trajectory (this

assumes that the

angle

0

should not be too

large

m order to prevent the

sphere

from

jumping).

In this scheme, the details

of the contact force between the moving

sphere

and the surface

spheres

are

unimportant.

However, one can assume

sufficiently large

friction to make sure that the

rolhng sphere strictly

follows the

edges

of the Voronoi

polygons,

m

particular

when it reaches a vertex where it has to

change

its direction quasi

instantaneously. Consequently,

m

projection

on P, the

trajectory

of the center of the

larger sphere

is made of successive segments which are all

edges

of

Voronoi cells

[12]

of the RSA

configuration

of the small

spheres. Figure

4 shows the Voronoi cells

corresponding

to the

configuration

of

figure

3.

2. Static results :

stability

threshold.

We studied 0~, the «

stability

» threshold first : it defines the limit of

stability

of a grain on the

surface,

and

depends

on the disorder of the 2D

packing

stuck on the

plane

and on the

smoothness 4l.

(5)

Fig. 3.

Fig.

4.

Fig. 3. A typical RSA

configuration

obtainetl by numerical simulations with C

= 0.52 (L

= 180 J

Fig. 4. Set of Voronoi ce[ls correspontling to the RSA

configuration

~hown m figure 3.

Consider first the

problem

from a theoretical and numencal point of view in two dimensions.

At each vertex, i-e- at each

point

i common to three Voronoi cells, where the

langer sphere

i~ in

contact with three smaller

spheres

of centers A, B, C (see

Fig. 5),

the

large ~phere

has to

choo~e its way

according

to steepest descent rules. This can be determined

by ca[cu[ating,

at

the vertex point, the

respective slopes

of the

possible

further

trajectofies

of the

large

ball

center. Let us calculate this

slope

for the motion in contact with

spheres

A and B. We call x the

unit vector

defimng

the steepest descent on P, y the unit vector

defining

the

in-plane

horizontal

direction, and z

= x x y

perpendicular

to P. In

projection

on P, the direction of motion i~

defined

by

a unit vector u,

perpendicular

to the segment AB. The unit vector t tangent, at the

vertex point, the further

trajectory

of the

large

bail center, is given

by

t = Cos qJu + sin ~Rz

z

~ t

tan~'zj

rll+©1

L ~ C

ti

Fig.

(6)

where the

angle

~R, indicated in

figure 5,

is

given by

~~~ ~

N/(l

+

~)2

r~ p~

~~

where h is the distance between the vertex point and the segment

AB,

and p is the radius of the circle which is circumscribed

by

ABC. As a function of x, y and z, t is given

by

t = u~ Cos ~Rx + u~ cas ~Ry + sin ~Rz

(2)

and,

using

now the «

laboratory

» set of unit vectors X, y and Z

(X being

horizontal and Z

vertical),

it is

given by

t =

(u~

Cos ~R Cos à + sm ~R sin 0

)

X + uy Cos ~Ry +

(-

u~ Cos ~R sin à + sin

~R Cos 0 Z

(3)

Consequently

the

slope

a~ of t is

given by

u~ cos ~R sin 0 + sin

~R Cos 0

a~ =

(4)

u~ cos ~R cos 0 + sin q~ sm 0

Une can write

tx~ = tan

(&

à

) (5)

with

tan &

= tan ~R

(6)

u~

8

might

be

mterpreted

as a local threshold

angle.

If the actual inclination ois

larger

than

8,

the

rolhng sphere

can roll over AB.

Using

equation

(I)

and h

=

iu,

where 1 is the

algebraic length

of iL

(see Fig. 5),

one gets

tan &

~/~i

+

~~

~.~

~~

~7)

If it is released at the vertex

point

without kinetic energy, the

Iarger sphere

is able to roll over

AB if a~ SO, 1-e- if MS 0. At each vertex i, we define r~ as

being

the minimum of

tan

Mi,

tan

8~,

tan

8~,

where

Mi, 8~, 8~

are the three

possible angles

8

(rolhng

over AB, BC

or

CA).

If r~ is smaller than tan 0, a

large sphere

released at vertex without kinetic energy will roll

naturally

on the

couple

of small

spheres

which

correspond

to the minimum

angle

8. If r~ is

Iarger

than tan 0, the vertex i

corresponds

to a stable

position

of the

large sphere.

In

figure 6,

we have

represented

all the

steepest

descent

trajectories

starting from all the vertices

(they

are the true

trajectories

for tan 0 m max~ r~. For smaller 0 values,

only

some of these

trajectories

are

actually

used smce the

rolling

hall can be

trapped

at some

vertices). They

look like a network of rivers and tributaries with main avers closed on to themselves due to

penodic boundary

conditions.

In our numerical

calculations, starting

from an initial RSA

configuration

we have

determined the

r,'s corresponding

to all vertices of the

corresponding

Voronoi network. Then

we have calculated the

quantity p(0 )

which

corresponds

to the fraction of r~ values smaller than a given tan 0. When comparing with an experiment,

p(0

also represents the fraction of balls which are able to move when

they

are released

anywhere

on P without initial kinetic

energy. It is easy to define

stability

thresholds from these distributions : it is the

angle

for which

p(0)

=

0.5,

as m the experiment. The results are given in

figure

7. Une notices that

p(0

does net staff from p =

0 for 0

=

0. This is due to the existence of some vertices which

(7)

Fig.

6. Ail ~teepe,t descent trajectories on Voronoi cell

edge~

for the RSA configuration ,hown in figure 3.

° lt/r=2

~

. lt/r=4 Ù,4

,

° lt/r=16

0,2

0 10 20 30 40 50 60

8

Fig. 7. Curves giving p(0) as a function of à.

are «

naturally

» un~table, even for

= 0 such vertices are located outside their

carre,ponding

ABC

triangles.

All the results that are

reported

here have been obtained with L

=

1801.

However, we have

performed

other calculation~ with different L values and we ha,,e checketl that for such

large

~ystems, the numefical results are quite

mdependent

on the size as fat a~ we stay

sufficiently

close to the

jamming

threshold.

Experimentally,

H, is determmed on average as follows : at each experiment, 50 stee[

spheres

(with diameters very well defined) are

placed

on the top of the (horizontal)

plane,

each of them

being

in stable

equilibrium

m a « cavity » formed

by

three smal[

glass sphere~

in

contact. This

explams

that is is not

possible

to

explore expenmentally

the non-stable situations

descfibed

just

above : we must start with 50 halls in stable

equflibrium.

From this initial situation, ois

progressively increased,

until one

sphere

moves, and falls down

along

the

plane,

and so on until all the 50

spheres

are down, the expenment is done again.

Finally, by

summing

six expenments (300

halls),

we have a

(Gaussian)

distribution of limit

equi[ibrium angles.

(8)

Figure

8

gives

this distribution for

4l=4,

and r=0.25 mm the mean value defines ô~. This distribution becomes wider antl wider when the smoothness

decreases,

as shown in

figure

9 which gwes the standard deviation of these distributions versus the smoothness

4l,

in a

log-log plot,

for r = 0.25 mm, r

=

0.5 mm and r

= mm.

N ' r=lmm

° Î ° r=0,smm

é'oà

° r=0~25mm

. @

O

~

0 10 20 30 40 1 10 ioo

O

Fig.

8.

Fig.

9.

Fig.

8. Distribution of the

stability angle

(~P = 4, antl r

= 0.25 mm) as the resu[t of six elementary experiments (300 balls).

Fig.

9. Variations of the standartl-tleviation of the distribution of the static angle with the smoothness

~P.

Figure

10 shows m a

log-log plot

the variation of H~

(normalized by

its value for 4l

=

2)

versus the smoothness 4l.

Experimental

and numencal values are well fitted

by

a unique curve

corresponding

to a power law H~ oz 4l

~, with an effective exponent x =

0. 8. When companng

simulations with the expenments, the most

important approximation

appears to be the

~~i

° Exp (r = 0,25 mm)

' Exp (r = 0,5 mm)

- . Exp(r=lmm)

C~

,

. simulations (C

= 0,52)

~°' ~~o

a

° simulations (C = 0,59)

~ o ,

ce

j

W ° o

à $

o .

o

lo~

1o° 1o~ o~

m

Fig.

10.

Log-Log

plot of the variations of the stability thresholtl H~ (normahzetl by its value for ~fi 21 for tlifferent sizes of stuck balls (expenments) or

packing

fraction C on the

plane

(2D numencal

simulations). All the results coalesce on a smgle curve well fittetl by a power law H~ cc ~P~~ with an exponent x = 0.8 ± 0.05.

(9)

replacement

of the

rough plane by

an RSA

configuration.

When

devising

the

rough plane,

the

sticking

process is

certainly

more

complicated

thon the

simple

rules of the RSA model. In

particular

due to the

unphysical

constraints of the RSA model, we are limited to a

quite

low

concentration

(lower

thon

0.547)

while

expefimental

concentration is of order of 0.7. We have

also

perforrned

similar calculations

using

a more realistic RSA model. in which ~nme

restructuring

is allowed

[1?].

With such a model one con reach

higher

densities of small

spheres

since the

jamming

concentration is

larger

(C m 0.61). The values obtained are

only slightly

srnaller than the previous ones, but

collapse

on the Sartre curve when normalized

by H,(2)

as can be seen in

figure

10. Une can also believe that

finding

0.8 and not is due to the fact that we are in the zone in which corrections to

~caling

are important (and this zone grows

when the

packing

fraction increases), see

equation

(7).

Another

interesting

result concerns the maximum value z~

= tg H~, of the

T,'s,

to which

corresponds H~

such that pi = I for

m

H~.

Ii can be calculated

exactly

at the

jamming configuration

in the asymptotic hmit of an

infinitely large plane.

This should

corre~pond

to a

vertex with the

largest

p value, which is p

=

2 r at

jamming,

and with a

configuration

a; that

represented

in

figure

11, i&.here the

large sphere

should roll over a ~mal[

sphere ju~t

in front of it. Thus

=

2 r and one finds

T~ = tg

H~

= ~ j8)

, (4S -1)(4l + 3)

à

A

r r

x

c

Fig.

Il Sketch of a

configuration

correspontling to 7

= 7~.

Numerical simulations agree very well with this formula, but there are some differences with the experiment, whose results are

presented

in

figure

12

compared

to theoretical values. A

linear variation is also observed

expenmental[y,

but tan

H~

is not zero at the

ongin

if we

extrapolate

the

expenmental

results. This is due to the contribution of friction, and

eventually

of attractive interactions between the ball and the stuck

glass spheres (capillary

forces..

these forces ensure the

stability

of the hall on non-horizontal

plane

(smal[ H) even for infinite smoothness.

3.

Dynamical

behaviour,

phase diagram.

In the above section, we have defined a

stability

threshold H~. which is

completely

defined

by

static conditions,

mamly geometncal

ones. We are here concemed with a

global analysis

of the different

dynamica[

regimes, and on its

dependence

on the geometry, i-e- on the smoothness of the

plane.

In these expenments and in the lD numerica[ simulations, the bail is thrown on the

(10)

3

R/r

' D

~im.ÎÎ

, BIC

° . Exn(r

m 0.25 mm)

° Exn(rmO.Smm)

. . Exp (rm mm)

~

a N1Im.olm. ~

o 50 ioo iso o ~ ~~ ~~ ~~

~'~~"

~

Fig.

12.

Fig,

13.

Fig. 12, Variations of tg H~ versus 2/

,~

according

to

equation

(8). The

straight

fine is the theoretical

prediction.

Fig. 13. ID phase tliagram obtainetl from numencal simulations (for s 0).

plane

with a small initial kînetic energy : we use a

drawing

straw

weakly

inclined with respect

to the

plane

as

launching

ramp. The

length

necessary to

forget

this initial kinetic energy is found

experimentally

to be very small

compared

to the

plane length

(a few

centimeters).

We have to compare here the static threshold H~ with the

dynamic

threshold H~, which is defined in this section. But our

goal

is to give a

phase diagram

first

descnbing

the different

dynamical

behaviour of the ball on a

rough

surface or

hne,

with control parameters which are the

angle

and the smoothness of the surface 4l. The ID

(numencal)

and 2D

phase diagram

are obtained.

Figure

13 shows the 1D

phase diagram

for no disorder

(e

=

0).

The contact conditions in this

example

are the

following

: the coefficient of restitution in this simulation is 0.5. For small values of 4~

(~ 0.8),

the behaviour of the ball is

dependent

on its initial

velocity.

For 4~ ~ O.8, the

plane

is divided in three parts,

according

to the values of H. For small values of the inclination

angle (region A),

the motion is decelerated. For

angles roughly

between 5° and

15°,

a constant

velocity

motion is observed

(region B),

whereas for

larger angles (region D),

the ball

velocity

increases

leading

to motions in which steps are

larger

than the minimum one

defined

by

two

neighbounng

balls thus

leading

to

jumps.

The situation observed in 2D

experiments

is very

comparable. Figure

14

gives

the

phase

diagram

obtained, also with 4~ and as control parameters. In the A region, the motion is decelerated : the initial kinetic energy is

quickly

lost. In the B region, a constant

speed

is observed, but the mean free

path (see

the

quantitative

definition

below)

is smaller than the size of the table

(2 m)

: the ball stops on the

plane.

In the C region, the

speed

is constant, but the

mean free

path

is

larger

than the table

length.

In the D region,

comparable

to its

equivalent

in the lD

diagram,

the bail

jumps,

and the scale of the motion is

completely changed.

We are

essentially

concerned with the constant

speed

regime. A

complete analysis

of the

dynamics

of this

problem, including

statistical aspects, is

given

elsewhere

[7]. Briefly,

the motion is the result of a balance between the gravity force and a « viscous » force integrating

«

microscopic

» collisions : so, the differential

equation descnbing

the average

(1.e. neglecting fluctuations)

motion of the ball is identical to that of the Stokes sedimentation of a

sphere

m a

fluid. It is clear

expenmentally

that this stable motion is

suddenly stopped

(not

decelerated) by

a

large

hole m the stuck

packing. According

to this observation, if one wants to descnbe the behaviour of the ball

completely,

we must add to the constant motion

description

a

probabihty

(11)

e~a~

fllr 2,8 ~"a~

D @~a~~

a~

a~

z ~~am~

c ea~

w a~~

© @~

m~~

A

~

0 4 a 2 16 20 40 60 80 100

8 1*

Fig.

14.

Fig.

15.

Fig. 14. 2D phase tliagram obtained from experiments.

Fig.

15.

Semilog

plot of the cumulatetl distribution N

(1

m 1* j of the stoppmg distance (1.e. number of spheres whose stoppmg distance Î is

larger

than a given value

Î")

obtamed under the followmg

conditions R

= mm, 1 = 0.25 mm,

= 4.7°, total number of spheres : 300.

for the ball to be

trapped

in a well. This

probabihty

is the same

everywhere

on the

plane

since it

is

supposed

to be

homogeneous,

and as a consequence, the distribution of the stoppmg distance

1 (projection

of the distance covered

by

the ball before

stopping

on the

largest slope line)

for

given

values of and 4l must be

exponential.

This is what we observe, as shown in

figure

15. which is a

semilog plot

of the cumulated distribution of

1.

The model descnbed

just

above allows us to make some

quantitative predictions

concemmg

the

dynamical

parameters

[7].

The mean

velocity

is

given by

~~

~~(ÎÎ

~ ~~~

where

f)

is the mean value of the

(fluctuating)

Stokes constant, and m the mass of the

rolhng

ball. We find that

(f)

varies with 4l as 4~+~~~.

Combining

the observed Stokes motion of the ball, and the use of extreme statistics to

analyse

the effects of traps on

1,

we propose

[7]

the

following expression

for the mean free

path

L on the

plane,

defined as the average

characteristic value

of1

determined from distributions similar to that shown m

figure15 (L

~

(i)

L

(H,

4l =

Lo

e~~~ =

Lo e~'

~~~~~~~

(10)

Table I

gives

different values of this mean free

path

L obtained from different values of and of the smoothness 4l. It shows in

particular

the very strong

dependence

of L on the

angle

and the

smoothness 4l: half a

degree

is sufficient to

multiply

L

by

5

Starting

from the distributions of the stoppmg distance

1,

we also define the

dynamical

threshold H~ as

being

the

angle

for which half of the balls have a stoppmg distance

larger

than the

plane length. Figure16

shows the variations of H~

(norrnahzed by

its value for 4l

=

2)

»eisus the smoothness 4l, for three different values of r. The three curves coalesce m a well

defined power law H~ =

4l~",

where y

=

1.55 ± 0.05.

Finally,

it is clear that H~ is

always

larger

than H~.

(12)

Table I.

Dijfierent

values

of

the mean

free path

obtained

f>.om dijfierent

values

of

and

of

the smaothness 4l,

expi"essed

in cm. The table

Îength

is 200 cm.

4l

(°)

4 5 6 8 lO

31

1,3 29 95

1,7 136 ~ 200

2 45

~ 200

2,5 18 139

3 81

~ 200

3,5

10 ~200

4 54

4,5 143

5 ~ 200

,~i

o

,o° o " ~*o,25mm

~

° r= O,5 mm

. * rm mm

m .

'

10'

~ o

4l

Fig. 16.

Log-log

plot givmg the variations of the dynamic threshold (normalized by its value for

~P

= 2) ver.sus the smoothness for three values of r.

4. Conclusion.

Surface

phenomena

are of great

importance

m

rapid granular

flow. This paper is a contribution to basic

understanding

of what are the relevant parameters in the motion of

partiales

on the

surface of a «

sandpile

», with a

particular

attention to segregation effects

by

surface flow. The

(13)

results obtained here outline the fact that on a

rough surface,

and

especially

on the surface of a

sandpile,

the

equîhbrium

and the motion of one

grain

is very

dependent

on its size

compared

to the surface

roughness.

The extreme

dependence

of the different thresholds and of the mean free

path

on the size of the

partiale

is at the

origin

of surface

segregation

: even if our results are obtained for mdividual

partiales, they explain why

the

large grains

are at the bottom of the

pile (not trapped by roughness),

as observed

by

numerical simulations

by

one of us

[2].

These

results must be

completed by

a more accurate

analysis

of the

dynamical

behaviour of

spheres

on a

rough

surface, and of collective

effects,

now m progress at Rennes.

Acknowledgements.

We would like to

acknowledge

our

colleagues

of the

laboratory,

and S. Roux for very useful discussions. This work was

supported

in part

by

the CNRS ATP « Matériaux

Hétérogènes

»,

and

by

the

Groupement

de Recherche CNRS

«

Physique

des Milieux

Hétérogènes Complex-

es »

References

iii Savage S.,

Interparticle

percolation antl segregation in granular materais, m

Developments

m

Engineering

Mechamcs, A.P.S. Selvadurai Ed. (Elsevier Science Pub. B-V-, Amsterdam, 1987).

[2j Jullien R, antl Meakin P., Nature 344 (1990) 425.

[3] Williams J. C., Chem. Froc.

Sup. (Apnl,

1965).

[4] Lebec F., Ristow G.antl Bitleau D., in preparation.

[5] Jaeger H. M. and Nagel S., Science 255 (1992) 1523.

[6] Lee J. and Herrmann H. J., J. Phys. A (1993) 373.

[7j

Rigmdel

F.-X., Hansen A. and Bitleau D., Earophys. Lent., to be submitted.

[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] Gervois A. and Bideau D., Hard disc

packings

some

geometncal

properties, m Disorder and Granular Media, D. Bideau and A. Hansen Eds. (Noah Holland, 1993).

[10j Ristow G. H., J. Phys. J Fiance 2 (1992) 649.

[1Ii Allen M. P, and Tildesley D. J., Computer simulations of

liquids

(Clarendon press, Oxford, 1987).

[12] Feder J. and Giaever I., J. Coll. Jnt. Sci. 78 (1980) 144 ; Feder J., J. Theor. Biot. 87 (1980) 237.

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