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HAL Id: jpa-00247479

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Packing at Random in Curved Space and Frustration: a Numerical Study

Rémi Jullien, Jean-François Sadoc, Rémy Mosseri

To cite this version:

Rémi Jullien, Jean-François Sadoc, Rémy Mosseri. Packing at Random in Curved Space and Frus- tration: a Numerical Study. Journal de Physique I, EDP Sciences, 1997, 7 (12), pp.1677-1692.

�10.1051/jp1:1997162�. �jpa-00247479�

(2)

Packing at Random in Curved Space and Frustration:

a

Numerical Study

R4mi Jullien

(~,*), Jean~franqois Sadoc (~)

and

Rdmy

Mosseri

(~)

(~) Laboratoire des

Verres,

Universit6

Montpellier

II, Place

EugAne Bataillon,

34095

Montpellier

Cedex 5, France

(~) Laboratoire de

Physique

des

Solides,

Universit6 Paris~sud, Centre

d'orsay,

91405

Orsay

Cedex. France

(~)

Groupe

de

Physique

des

Solides,

Universit6 Paris VII, Place Jussieu.

75251 Paris Cedex 05, France

(Received

3

July

1997, received in final form 11

August

1997,

accepted

18

August J997)

PACS.61.43.Bn Structural

modeling:

serial-addition models, computer simulation PACS.61.20.Ja

Computer

simulation of

liquid

structure

PACS.61.72.~y

Defects and impurities in

crystals;

microstructure

Abstract. Random

packings

of discs on the

sphere

52 and

spheres

on the

(hyper~)sphere

53 have been built on a computer using an extension of the

Jodrey~Tory algorithm.

Structural

quantities such as the volume fraction, the pair correlation function and some mean character~

istics of the Voronoi cells have been calculated for various

packings

containing up to N

= 8192

units. While the disc

packings

on 52 converge

continuously,

but very

slowly,

to the

regular

trian~

gular lattice,

the

sphere packings

on 53 converge to the disordered frustrated Bemal's

packing,

of volume fraction c ~ 0.645, in the

(N

=

cc)

flat space limit. In the 53 case, the volume

fraction exhibits maxima for

particular

values of N, for which the

corresponding packings

have

a narrower

histogram

for the number of

edges

of Voronoi

polyhedra

faces.

1. Introduction

Random

packings

of identical hard

spheres

in three dimensions have been used

throughout

the last decades to

represent

the structure of

liquids, amorphous

solids or

glasses [1-6].

Since the

pioneering

work of Bernal

iii

it is known that the volume fraction of a random

packing

of

spheres

cannot exceed a limited value of cb " 0.645

significantly

smaller than the

packing

fraction 0.7405 of the most

compact regular

structures

(face~centered~cubic

and

hexagonaL closed~packed)

in three

dimensions,

in contrast with the two~dimensional case where the sur~

face fraction of the

triangular

lattice of discs

(0.907)

can be reached

continuously.

It is now believed that this

property

is due to the so~called

geometrical

"frustration" associated with the

impossibility

to tile the d

= 3 space with identical

perfect

tetrahedra

only [7-9]

while the

plane

can be tiled with identical

perfect triangles.

A way to vary, and sometimes

eliminate,

frustra~

tion is to consider curved spaces. The recent

investigations

of atomic

arrangements

in curved spaces has been proven to be very

useful, mainly

for the

understanding

of disordered materials and

quasicrystals [8,9],

but also for the

study

of

systems

with

long

range interactions

[10]-

(*)

Author for correspondence

(e~mail: remislldv.univ~montp2.fr)

@

Les

#ditions

de

Physique

1997

(3)

In this paper, we

investigate numerically

the

geometrical properties

of random

packings

of

spheres

built in a curved space of constant

positive

curvature, I-e- the

"sphere 53".

Such a

space is the extension to one dimension more than the standard

sphere,

the

sphere 52. Indeed,

discs

packings

on the

sphere 52

have also been

investigated

for the purpose of

comparison.

It is worth

mentioning

that the

problem

of

packing

discs with the maximal volume fraction on a

sphere

has

already

been

investigated ii Ii

and is very close to the old Thomson

problem

which

consists in

finding

the most stable

configuration

of a set of

equal charges (by minimizing

the Coulomb

energy) [12].

Our

packings

have been

analysed by calculating

their

pair

correlation functions and

by characterizing

the statistics of their "Voronoi cells". We recall that the Voronoi cell for one

sphere

is the

region

of space closer to that

sphere

center than to all other

sphere

centers.

Knowledge

of the Voronoi cells has proven to be very useful in the

analysis

of local

geometrical properties

of random

packings

[2]- Not

only

have we extended to curved space an efficient

algorithm

introduced

by Jodrey

and

Tory [13]

to generate the

packings

but also the methods of calculation for both the

pair

correlation function and the Voronoi tessellation. In that

framework the

present

work can be considered as an extension of a recent paper in which

large sphere packings

were studied in the Euclidian d

= 3 space

[14, lsj.

Smaller

packings

have

previously

been built on

53

but with other

algorithms dealing

either with soft

[16]

or hard

ii?]

spheres.

In Section

2,

we describe the

principles

of the numerical

methods,

in Section 3 we present and discuss the results and in Section 4 we conclude.

2.

Principles

of the Numerical Methods

2.I. GENERALITIES. Since

they

are very

similar,

we will

present together

the numerical methods that we have used to build and

analyse

the discs

packings

on

52

and the

sphere packings

on

53.

For

simplicity

we will

speak

in both cases of

'~spheres"

and

"volume",

even

if,

in the case of

52,

this means "discs" and "surface". When

working

on

Sd-i,

we are

considering

the

sphere

centers as a set of N

points

M~

(I

=

1, 2,

,

N),

in a d~dimensional Euclidian space

(d

= 3 or

4),

such that their distance to the

origin

is

equal

to a constant R which is the radius of curvature of the

spherical

space.

Introducing

the coordinates x~k

(k

=

1, 2,.-, d)

of the

vector r~ =

OM~,

this reads:

'~~'~

"

~

X~k

~

~~. (~)

k

The

expression

for the

"geodesic"

distance d~j between two

points

M~ and

Mj (I-e-

the shortest distance counted

along

the curved

space)

is

simply

related to the scalar

product

of r~ and rj:

d~j =

Rcos~~

~~

)~

=

Rcos~~ ~~

~(~~~ (2)

R R

The volume of a

sphere

of radius r can be

expressed

as a function of uJ

= r

/R,

u(uJ)

=

2~(1 cosuJ)R~ (52) (3a)

u(uJ)

=

2~(uJ "j")R~ (53) (3b)

as

depending

whether one is

working

on

52

or

53.

As a consequence, the volume

fraction,

also called

"packing fraction",

c, of a

packing

made of N

spheres

of diameter

do

is

equal

to the total volume

occupied by

the

spheres,

which is

Nu(do/2R),

divided

by

the total volume of

Sd-1,

(4)

which is

u(~).

Therefore:

c =

~

(l cosuJo) (52) (4a)

2

~

~"° ~~~~~

~~~ ~~~~

with:

~

"o #

). (5)

It is worth

noticing

that one recovers the well known

expressions

for the definition of the distance and for the

packing

fraction in the limit

R/do

~ cc of a flat space.

2.2. EXTENSION oF THE JT ALGORITHM. We recall that the

Jodrey-Tory (JT) [13]

aI~

gorithm

is an iterative method in which a set of N

points

is modified

sequentially

in order

that two chwcifistic

(geodesic) di§fhncwdxi

and

dj~(dfim)~

WA

don#ergiq

tithe fibhl

sphere

diameter

do Considering

the N

points

as centers of

spheres

of diameter

dm,

or

dM,

one

gets packings

of

non~overlapping,

or

overlapping, spheres, respectively,

with

packing

fractions cm < cM. The distance

dm always corresponds

to the lowest distance between

pairs

of

points

while the distance

dM

is set to an initial value

d[

and is

continuously

decreased

along

the iterations

according

to a rule which will be

given

below. The initial set of

points

is chosen

randomly

and

uniformly

in the available space.

The method that we have used to

generate

the initial set

depends

on the space dimension.

In the case of

52,

we consider the standard

(polar coordinates) parametrization

of a

sphere

in the Euclidian 3d space:

xi #

Rsinbcos#;

x2

# R sin b sin

#;

x3

# Rcosb

(6a)

where b runs from 0 to ~ while

#

runs from 0 to 2~.

According

to the

expression

of the

elementary

solid

angle:

d~Q

= sin

bdbd#

=

-d(cos b)d# (7a)

one can build a uniform random distribution of

points

on

52 by choosing,

for each

point,

a value for cos b

uniformly

at random between -I and +I and for

#

between 0 and 2~- In

practice

we

use:

fi

=

cos~~(1 2fi)I

§i

~

2~f2 (8~)

where

fi

and

f2

are two

independent computer generated

random numbers

uniformly

dis- tributed between 0 and I. The same kind of

procedure

has been used on

53 except that,

for

convenience,

we have used the

following parametrization (which

is not a

straightforward

exten~

sion to 4d of the

spherical

coordinates of

equation (6a),

but rather "toroidal" coordinates

[9]):

xi " R cos b cos

#;

x2

" R sin b cos

#;

z3

~ R cos ifi sin

#;

z4

~ R sin ifi sin

# (fib)

where the

angles #,

b and ifi run from 0 to

~/2,

2~ and

2~, respectively.

The

elementary

solid

angle

is then:

d~Q

= sin

#cos # d#dbdifi

=

~d(sin~ #)dbdifi. (7b)

2

Accordingly

we

take,

for each

point:

#

=

sin~~ fit

b

=

2~f2i

~fi #

2~f3 (8b)

where the

f~'s

are random variables between 0 and 1.

(5)

Then the JT

algorithm proceeds

as follows. At each step of the iteration

(p)

the two

points Mi

and

M2

at shortest distance

dk~

are identified.

They

are then

pushed

apart

symmetrically

in the direction

MiM2

so that their new distance is

equal

to

d$~.

To do so, one first determines the coordinates of the mid

point

C of

MiM21

rc # R ~~ ~ ~~

(9)

ri + r2 The new

position M[

of

Mi,

is

given by:

~~~~~

rc ri

di~

~ ~

(11)

R2 ' ~ ~°~ 2R

one can determine ~

by:

c~/(1 s2)(1 c2) ii s)(1 c2)

~

~

ii

S)12C~ + S

1)

~~~~

The new

position M[

of

M2

is determined

similarly. Then,

before

going

to the next

iteration,

the distance

dM

is decreased

according

to:

dj~~~~

= dj~~

~

(cj~~

c~f~)" (13)

where

c(~

and c~f~ are the

packing

fractions associated with

d(~

and d~f~

through

formulae

(4, 5)

and where the parameter K and the

exponent

a are two

input parameters

of the al-

gorithm.

Note that we have used

here,

as in reference

[14],

a

simpler

formula than the one

initially

introduced

by

JT

[13j-

The process stops at the iteration step

(n)

when one gets

d~~

< d~0~- Then

db~

becomes the actual

sphere

diameter

do

for the

resulting packing.

2.3. SOME TECHNICAL POINTS. The

input

parameters of the computer code are

R, N,

d(,

K and a. Note that the value taken for the space radius R does not

play

any role since it fixes

only

the unit of

length.

A more

important parameter

is N which fixes the size of the

packing.

In the limit of

infinitely large N,

the

resulting sphere

diameter

do

tends to zero. In the

following,

all the

lengths

will be counted in units of the

sphere diameter,

and therefore R will stand for

R/do. Consequently

the limit N ~ cc

corresponds

to the limit R ~ cc of

an

infinitely large,

and

flat,

space. The choice for the value of

d~~

is not very

important.

It should be

sufficiently large

however to

guarantee

that

spheres

of diameter

d~~

would

overlap.

In

practice,

we take:

d~J

=

2Rcos~~(1 j) (52) (14a)

d(~

=

2R(

~~

)i (53). (14b)

This choice

corresponds

to

c(~

= l in the case of

52,

as in the

original

paper of JT

[13j,

and

c~~

very close to I in the case of

53.

The

remaining

parameters K and a are essential not

only

to fix the final

packing fraction,

but also to determine the rate at which it is reached. For

given

(6)

a, the smaller

K,

the

larger

the

resulting packing fraction,

but the

longer

the

computation

time. Also the

larger

N

is,

the smaller K must be to

get

the same accuracy on the

resulting

volume fraction. Here we have taken o

= 0.5 and 0.33 in the case of

52

and

53, respectively

and in most of the calculations

reported

below we have taken K

=

10~~

Note that the set of parameters used on

53 corresponds

to the one used in a recent calculation in the Euclidian

d = 3 space were the Bernal's volume fraction was recovered within more than 0.I per cent

accuracy for

packings containing

N

= 8192

spheres [14j-

Some tricks have been used to

optimize

the JT code and there is no need to describe them in

great

details here. In

particular

the search for the

pair

of

points

at minimum distance is

optimized by updating

at each iteration a list of distances in

increasing

order

together

with

a table to recover the

particles

for any

pair

on the list. Also the search for

points

in the

neighborhood

of another one is accelerated

by using

an

underlying hypercubic

lattice in the d-dimensional space which defines

(hyper)boxes

used to locate and label the

sphere

centers.

To

give

an

idea, generating

a

packing

of 8192

particles

on

53

with K

=

10~~

takes

a few hours of IBM RISC

6000/380 computer

time.

2.4. PAIR CORRELATION FUNCTION AND VORONOI TESSELLATION. After a

packing

has

been constructed it is characterized

by calculating

its

pair~correlation

function

g(r)

and

by performing

a Voronoi tessellation. The

pair~correlation

function, which is

proportional

to the

probability

to find a

point

at a distance r from a

given point

and which is normalized to

unity

for infinite r, is calculated

by using

the formula:

gin)

=

(jlUo

~~~~

where dN is the number of

points

located in the volume du

corresponding

to distances between

r and r + dr from a

given point

and uo is the volume of an individual

sphere.

The presence of

c in the denominator ensures that

g(r)

= I when

considering dN/du

=

N/u(~)- Introducing

uJo #

do/2R

and uJ

=

r/R,

this formula becomes:

~~~~

~

c

i~~~

~

~~~~ ~~~~~

~~~~

~

~~

2c

~ii~~~~

~ ~~~~ ~~~~~

In

practice

we have considered dr

= 0.05 in diameter units and dN has been

averaged

over all the

points

of the set.

To

perform

the Voronoi

tessellation,

we have extended to curved space an efficient

algorithm

which has been described in reference

[14].

We have first determined the

"simplicial cells",

which are

triangles

on

52 (resp.

tetrahedra on

53),

which are, among all the ensembles of three

(resp- four) points,

those such that no other

point

of the set lies inside their circumscribed circle

(resp. sphere). By

circumscribed circle

(resp. sphere)

we mean the set of

points

which

are at the same

geodesic

distance from a

given point

Q as the three

(four) points.

To do so,

one should be able to find the center Q of the circle

(resp- sphere)

circumscribed to a

triangle MiM2M3 (resp.

tetrahedron

MiM2M3M4). Defining

the

~~'s by:

d

rn =

~j [r~ (17)

~=1

they

must

satisfy

the set of d

equations:

~j

~~r~ rj

=

R~

cos

~~ (18)

R

(7)

Fig.

1- Two-dimensional projections of disc

packings

on 52 with N values

ranging

from 4

(top left)

to 12

(bottom right)-

The

projections

of the discs centers are indicated

by

white dots or black dots

(in

the case of

multiple projections)

and the bonds

(corresponding

to

simplicial

cell

edges)

are

represented by straight

line segments instead of ellipses arcs. Back lines are dashed.

where

Rn

is the unknown circle

(resp. sphere)

radius. This is done

by using

standard linear inversion

computer procedures.

After the

simplicial

cells have been determined the construction of the Voronoi cells becomes trivial if one knows that the

simplicial

cells

edges correspond

to

Voronoi cell

edges (resp- faces)

and that the Q's are Voronoi cell vertices. In

particular

the number of

edges (resp, faces)

of a Voronoi cell

surrounding

a

given point

is

equal

to the number of

simplicial

cell

edges

connected to this

point. Moreover,

in the case of

53,

the number of

edges

of a face is

equal

to the number of

simplicial

tetrahedra

having

a common

edge,

which is the

corresponding

nearest

neighbor

distance. We have written a code that reads the list of

point

coordinates and

produces

the fractions

fe

of cells with

e~edges,

in the case of

52,

and both the fractions

fF

of cells

having

F faces and the fractions

fe

of faces

having

e

edges,

in the case of

53.

3. Numerical Results

3.I. EXAMPLES FOR SMALL N. It is

quite

easy to vizualize the discs

packings

obtained

on

52

and we

provide

some

typical examples

obtained for values of N

ranging

from 4 to

12,

in

Figure

I. The

corresponding

values of the

packing fraction,

the radius of the space in diameter

units,

the mean coordination numbers z, and the fractions

fe

of Voronoi cells

having

e

edges,

have been

reported

in Table I- In the

figure

we

represent

the horizontal

projections

on the

plane (xi, x2)

after

having performed,

for each

packing,

the

adequate

rotation of the

sphere 52

to get a

point

on the north

pole (x3

~

R)

whose

projection

is therefore

always

located at the center of the

figures.

The

projections

of discs centers are

represented by

white dots

(or

black

(8)

Table I- Radius R

of

the

sphere 52 (in

disc diameter

unit), packing fraction

c, coordination number z, and

fraction fe of

Voronoi cells with e

edges for packings of

discs on

52

with values

of

N

ranging from $

to le.

N R c Z

f3 f4 f5 f6

4 0.523 0.8453 3 1 0 0 0

5 0.637 0.7322 3.6 0.4 0-6 0 0

6 0.637 0.8787 4 0 1 0 0

7 0.736 0.7774 4.285 0.142 0.428 0.428 0

8 0.765 0.8236 4-5 0 0-5 0.5 0

9 0.812 0.8258 4.667 0 0.333 0.667 0

10 0.866 0.8101 4-8 0 0.2 0.8 0

II 0.903 0.8214 4.909 0 0,182 0.727 0-091

12 0.903 0.8960 5 0 0 1 0

dots when

they correspond

to two discs

centers)

and the bonds

connecting

nearest

neighbors (edges

of

simplicial triangles)

are

represented by straightlines

instead of arcs of

ellipses.

It is worth

noticing

that most of the

configurations depicted

here are

quite symmetric

and are not

truly

"random". In

fact,

for such small N values

(except

for N

=

5),

the

topology

of the final

configuration

does not

depend

on the choice of the initial random

configuration.

This is no

longer

verified for

large

N values as it will be discussed below.

Anyway

the most ordered and

symmetric

structures

correspond

to the

largest

values for the

packing

fractions. In

particular,

in the cases N

= 4

(top left),

6

(top right),

12

(bottom right),

the

points

are located at the vertices of the

only existing perfect polyhedra

made with

perfect triangular faces,

which are

tetrahedron,

octahedron and

icosahedron,

with

integer

coordination numbers z

=

3,4

and

5,

respectively,

and with

fe

= 0 for e

#

z and

fe

= I for e

= z. The

corresponding packing

fractions are c

=

0.845,

0.879 and 0.896.

They extrapolate nicely

to the

trianglar

lattice which

corresponds

to N

= cc, z = 6 and c

=

0.907. All the other cases exhibit much less

symmetry

and have a broader distribution of

fe's.

For

example,

in both cases N

= 5 and N

=

II,

the

structure-corresponds

to a

perfect polyhedron

with a vacancy. Note that in the case N

= 5

(at

the top center of

Fig. I)

there is a "continuous

degeneracy"

since the three

points (white dots),

which are not on the north and south

poles (black dot),

are free to rotate around them

(within

hard core

constrains).

The case N

= 8

(at

the center of

Fig, I)

is

tricky

since the

points

are not located on the vertices of a

perfect

cube.

They

reach a more compact structure

exhibiting only

two

parallel perfect

square

configurations

of

neighbors,

twisted

by

an

angle

of

~/8.

Note that these square

configurations

are

degenerate

in the sense that there are two different choices for the

simplicial triangles (our

code then

performs

an

arbitrary

choice for the

bonds).

Nevertheless the

configuration

is

unique.

It is worth

noticing

that all our smalLN

configurations

very often

correspond

to the ones

recently

obtained

numerically

for the

closely

related Thomson

problem [12j.

It is

obviously

less easy to vizualize the

sphere packings

on

53.

Given a

single plane projection

is

generally

not sufficient to

figure

out how the

points

are

organized. Anyway

the same trends

are observed: the more

compact

is the

packing,

the more

sylhmetric

is the

configuration

and the less rich are the

fF

and

fe

distributions. The

simplest

Voronoi

tessellations,

with identical

perfect polyhedral cells,

are obtained for N

=

5,

8 and

120,

where the values of z are

4,

6 and 12,

respectively.

The cells are

perfect

tetrahedra

IF

= 4, e =

3),

cubes

IF

=

6,

e =

4)

and

(9)

Fig. 2. Two-dimensional projections of sphere

packings

on 53 with N

= 5

(top left),

8

(top right),

120

(center

and

bottom).

The

projections

of the

sphere

centers are indicated by white dots or black dots

(in

the case of

multiple projections)

and the bonds are

represented by straight

line segments. In the case N

= 120, three different

projections

are shown.

Table II. Radius R

of

the

sphere 53 (in

disc diameter

unit), packing fraction

c, coordina- tion number z, number e

of edges of

Voronoi cells

faces, for packings of spheres

on

53

with N

=

5,

8, 120.

N R c z e

5 0.5484 0.6806 4 3

8 0.6366 0.7268 6 4

120 1.5915 0.7741 12 5

dodecahedra

(F

=

12,

e =

5)

and the

packing

fractions are

0.6806, 0.7268, 0.7741, respectively.

They correspond surely

to

polytopes (3, 3, 3), (3, 3, 4)

and

(3, 3, 5) using

the notation of Coxeter

[18j.

Two~dimensional

projections

of these

packings

are

represented

in

Figure

2 and the

corresponding

values of c and R are

reported

in Table II. For these

projections

we have

performed

rotations of

53

in order that two different

points

are

projected

at the center of the

figure.

As in

Figure I,

when two, or more,

sphere

centers have the same

projection, they

are

represented by

a black dot. Therefore the center

point

is

always

a black dot. Note that for N

= 8

(top right)

it

corresponds

to fur

sphere

centers. For N

= 120 one recovers the

so-called

polytope (3, 3, 5) [18,19j

which exhibits five~fold

symmetry

and

corresponds

to the most compact

packing.

In

Figure

2, we have

represented

three different

possible projections

of

polytope (3, 3, 5)

which exhibit

symmetry 10,

6 and 4. Note that its volume fraction is

larger

than the one of face-centered~cubic and

hexagonaLclose-compact

structures in flat space.

(10)

o.95

o.90

0.85

0.80

0.75

0.70

II .(j/

'

0.65 II ;.

.>I'/l~~ l~~',

',"

..

" ....°

o.60

~ ~~ loo iso 2°° ~~° ~~~

N

Fig.

3. Numerical results for the packing fraction c as a function of N up to N

= 300 in both the

52

(upper curve)

and 53

(lower curve)

cases. Five independent results have been recorded for each N value.

3.2. RESULTS FOR INTERMEDIATE N VALUES. The numerical results for the

packing

fraction c for N values up to 300 are

depicted

in

Figure

3 for both the

52

and

53

cases. We have run the code five times for each value of N

using independent

seeds for the random

generator. Despite

some noise which can be attributed to both the lack of

efficiency

of the

algorithm (in

the

figure

we have taken a

= 0.33 and K

=

10~~,

as

explained above)

and the randomness of the initial

configuration,

the "curves"

c(N)

turn out to be

qualitatively

different

in the two cases, at least in the range of N values

reported

in the

figure.

In the

52

case, the

dispersion

of the

points, already

found for the small N values discussed

above, disappears progressively

as N increases while the mean c~value increases very

slowly

from c cf 0.835 for N = 100 to N m 0.845 for N

=

300,

a value still

significantly

smaller than the

packing

fraction 0.907 of the

triangular

lattice.

In the

53

case, the

dispersion

of

points

turns out to be such that one can define

roughly

two different mean curves. The lower curve is almost flat and

corresponds

to a c~value of about

0.655,

close to

(and slightly larger than)

the Bernal's

packing fraction,

while the upper curve exhibits a series of maxima. We will comment more on these two curves later

(Sect. 3.4)

but

we would like first to focus on the maxima of the upper curve.

They

are

asymetric

in N since it is easier to create a vacancy than to add an extra hard

sphere

to a

compact

structure. In

particular,

all the most

compact

structures obtained from N

= III to N

= l19 turn out to

be the

polytope (3, 3, 5)

with a

given

number of vacancies. As a consequence the upper

c(N)

curve is linear in that range of values of N.

Moreover,

as was

already

noticed on

52

for small

values of

N,

we observe that the maxima

always correspond

to the more

regular

structures with

narrower distributions for the

fe's.

This is

obviously

the case of the

sharp peak

at N

= 120

(11)

.o

0.8 O 75

~ . 76

u 77 o

u 0.6

0A

O.2

~ O

O-O

2 e

Fig.

4. Fraction of Voronoi cells faces with

e~edges, fe,

as a function of e for

spheres packings

on 53 with N

= 75

(open circles),

76

(filled circles)

and 77

(squares).

~

fiO

§

Q

fibCIJ~jJ

o

~o ~O

O

~

~ ~~ jfj

~~j~~jj~~li~

llJ

o~

°

cc O

Fig.

5. Two-dimensional projections of sphere

packings

on 53 with N

= 20 and 76 with the same

conventions as in

Figure

2. The bonds are not shown for N

= 76.

but this is also true for all the

secondary peaks.

To

give

an

example,

we have

reported

the

fe histogram

for the most compact

packings

obtained with N

=

75,

76 and

77,

in

Figure

4. As

one can see, these

histograms

are more

peaked

for N

= 76 which

corresponds

to a maximum

of the

c(N)

curve.

However,

for

larger

values of

N,

the

packings corresponding

to maxima

do not exhibit

special symmetries.

This is illustrated in

Figure

5 where we have shown the two~dimensional

projection

of the

packings

obtained for N

= 20 and N

=

76,

both of which

corresponding

to maxima of the curve. While the N

= 20

packing

exhibits some symmetry the N

= 76

packing

looks random. In both cases the Voronoi tessellation

only

involves two

topological

kinds of

cells, polyhedra

with 9

(fg

=

0.8)

and 10

(fir

=

0.2)

faces in the case

(12)

o.95

o.90

*

0.80

"

O.75 . lO"~

o.70

,

.65

O.60

~~

~~

~'~

l/N o.95

o.90

O.85

~ ° l

lo'~

o.75

o.70

,

O.65

.60

O.OO

.05 -lo .15 .20 .25

b)

Fig. 6. - Large N numerical results for K =

The packing

and

53

curve)

cases.

(13)

Fig.

7.

Stereographic

projections of

packings

of discs on 52 with N = 4096 and N

= 8192.

Only

the 1024 discs closest to the

projection

center have been

represented.

The discs with e

~

6 are indicated by black dots.

their

regularity (geometric progression)

rather than for any technical reasons. The results for the the

packing

fractions are

reported

as a

plot

of c versus I

IN

in

Figure

6a and versus

II log

N in

Figure

fib. In the

52

case the convergence to the

triangular

lattice does not show up in the I

IN plot

of

Figure

6a as well as in any

plot

of the type I

IN".

As seen in

Figure

fib the convergence to 0.907 is more

likely

of the

type II log N,

which is an

extremely

slow convergence.

To illustrate this slow convergence we have shown in

Figure

7 some

stereographic projections

of the

packings

obtained with N

= 4096 and N

= 8192. The

stereographic projection

is a standard

procedure

used in

cartography. Imagine

a north

pole

N and a south

pole

S. The

projection

M' of any

point

M of

52

is obtained

by intersecting

NM and the

plane tangent

to

52

in S. Such a

projection

has the

advantage

to transform circles into circles. In the

figure only

the 1024 discs closest to the south

pole

have been

represented

in both cases. Note that the effect of curvature, which is to increase the apparent diameter of the discs when

going

from the center to the

periphery

of the

projection,

is

hardly

visible on the

figures,

due to the

large

values of N. The discs centers

corresponding

to

defects,

I.e. to Voronoi cells with e

# 6,

are

indicated

by

black dots. These defects form

lines,

or

"grain boundaries",

whose

density

does not decrease

significantly

when

increasing

N. The

necessity

to

keep

an

homogeneous

array of

grain

boundaries as N increases is due to the constant curvature of the space.

In the

53

case the convergence to the Bernal's value is so

quick

that it can

already

be seen in the I

IN plot

of

Figure

6a.

Indeed,

there is no way to

imagine

a convergence to the fcc value.

The difference between the

52

and

53

cases can also be stressed on the

g(r)

curves

(Figs.

8a and

8b). While,

in the

52

case, one sees an evolution towards

sharp peaks

as N

increases,

as

it should be when

approaching

a

crystal,

this

sharpening

is absent in the

53

case. It is worth

noticing

that the

g(r)

curve obtained for N

= 8192 is

remarkably

close to the one

corresponding

to a Bernal's

packing

of the same number of

particles

built in a cubic box

[14j.

All the well known characteristic features are

present,

in

particular

the twin

peaks

at r =

v5

and

r = 2.

One sees in

Figure

8b that the

peak

at r

=

vi

results from

a shift to

larger

r of the second

neihgbor peak

of the

polytope (3, 3, 5).

The statistics of the Voronoi tessellation are also very similar to those for Bernal

packings.

In

Figure

9 we

give

the results for the coordination number z, which is the mean number of faces of the Voronoi

cells,

as a function of I

IN.

Note that there is an exact

relationship

between N and z in two dimensions

(z

=

6(1- 2/N)) [20j

which has been verified

by

our

numerical results. In three dimensions one

gets only

an

approximate

linear behavior in I

IN.

It is worth

noticing

that the

extrapolation

to N infinite

gives

z = 14.22 as the coordination number of the "ideal"

(infinite)

Bernal's

packing.

Such a value is consistent with values of z

(14)

5.o

4.O 256

8192

3.O

2.O

i .o

~'~0

2 3 4 5 6 7 8 9 lo

a)

r

3 0

I

I

t 128

2.5

II 256

Ii

8192

11

~ ~ /j

' l

# 5 '

1 ~

C'

/ ji

)

1.0 '

'

~~ Ii

0.5 ' ,'

O-o

0 2 3 4 5

b)

r

Fig.

8. Pair correlation functions

g(r)

for

packings

of discs on 52 with N = 256 and 8192

(a)

and for

packings

of spheres on 53 with N = 128, 256 and 8192

(b).

In

(b)

the delta

peaks

of the

g(r)

curve

for the

polytope (3,

3,

5) (N

=

120)

are shown with arbitrary units.

obtained from finite Bernal

packings

built in a cubic box

[14].

Note that other

algorithms

based on tetrahedra

packings (which

do not deal with hard

spheres)

lead to z values of about 13.4 [9,

21, 23]

in close connection with the statistical

honeycombs

of Coxeter

[22].

It would be

interesting

to understand whether these two values

(14.2

and

13.4)

are related.

(15)

14.5

14.0 13.5

~~'i.000 .001

1/N

(16)

400

300 128

256 512

)

200

loo /,

/ ,

'

'~-~

'

/ '

~

' 0

0.64 0.65 0.66 0.67 0.68

c

Fig.

10. Histogram of the

c values obtained when running the

Jodrey~Tory

code

fifty

times for

packings

of

spheres

on 53 with N

= 128, 256 and 512. All results have been obtained with K

=

10~~

converges

slowly

to the

triangular

lattice while the three~dimensional

sphere packing

converges

to the frustrated Bernal

packing.

For some

particular

values of the number of

spheres

the

packings

on

53

are more compact and exhibit narrower

histograms

for the Voronoi cells char~

acteristics. Such a

study presents

a way to understand the mechanisms of frustration in real disordered

systems.

It also

provides

an alternative way to reach the

thermodynamic

limit in numerical methods

deeling

with

large

three dimensional systems. Instead of

working

in a flat

space within a cube

subject

to

periodic boundary

conditions

(which

is

topologically equivalent

to

working

on a

torus),

and

trying

to reach the

thermodynamic

limit

by increasing

the

edge length

L of the

cube,

one can work on

53 by increasing

the space radius R. The geometry is

slightly

more

complicated geometry

but there are considerable

advantages.

In

particular

the space remains

isotropic

for all values of R. This

might

be an

advantage

in

studying glasses

for which it is well known that the

anisotropy

of the

boundary

conditions can induce artefactual

crystallization.

In the future we intend to

develop

numerical methods such as Monte~carlo or molecular

dynamics

to

study glasses

in curved space.

Acknowledgments

Numerical calculations were done at CNUSC

(Centre

National Universitaire Sud de

Calcul), Montpellier,

France. One of us

(R.J.)

would like to thank discussions with Didier

Caprion

and

Philippe

Jund.

References

iii

Bemal

J.,

Proc.

Roy.

Soc. A 280

(1964)

299.

[2]

Finney J-L-,

Proc.

Roy.

Soc. A 319

(1970)

479:

(17)

[3j Bennett

G.H.,

J.

Appl. Phys.

43

(1972)

2727.

[4j Adams D.J. and Matheson

A-J-,

J. Chem.

Phys.

56

(1972)

1989.

[5j

Cargill G.S.,

J.

Appl. Phys.

41

(1972)12.

[6j Bernal J.D. and Mason

J.,

Nature188

(1990)

910.

[7] Sadoc

J.F.,

Dixmier J. and Guinier

A.,

J-N- C-S- 12

(1973)

48.

[8j Sadoc F. and Mosseri

R.,

in

"Aperiodidicity

and order

3,

Extended icosahedral structures"

(Academic Press,

New

York, 1989)

p. 163.

[9j Mosseri R. and Sadoc

J-F-,

in

"Geometry

in condensed matter

physics",

Directions in Condensed Matter

Physics, 9,

J-F-

Sadoc,

Ed.

(World Scientific, Singapore, 1990)

239.

[10]

Delville

A., Pellenq

R-J-M- and Caillol

J-M-,

to appear in J. Chem.

Phys. (1997).

ill]

Troadec

J-P-,

Gervois

A.,

Bideau D. and

Oger L.,

J.

Phys.

C 20

(1987)

993.

[12]

Altschuler

E.L.,

Williams

T-J-,

Ratner

E.R.,

Dowla F. and Wooten

F., Phys.

Rev. Lett.

72

(1994)

2671.

[13] Jodrey

W.S. and

Tory E.M., Phys.

Rev. A 32

(1985)

2347.

[14]

Jullien

R.,

Jund

P., Caprion

D. and

Quitmann D., Phys.

Rev. E 54

(1996)

6035.

[15] Oger L.,

Gervois

A.,

Troadec J.P. and Rivier

N.,

Philos.

Mag.

74

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177.

[16] Straley J.P., Phys.

Rev. B 30

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6592.

[17j Mackay A.L.,

J.

Phys.

A 13

(1980)

3373.

[18j

Coxeter

H.S.M., Regular Polytopes (Dover, 1973).

[19j

Sadoc

J.F.,

J.N.C.S. 44

(1981)

1.

[20j

Rivier

N.,

in "Disorder and

granular media",

D. Bideau and A.

Hansen,

Eds.

(Elsevier

Science

Publishers,

North Holland~

1993)

p. 55.

[21j

Nelson D.R. and

Spaepen F.,

Sol. State

Phys.

42

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1.

[22j

Coxeter

H-S-M-,

Illinois J. Math. 2

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746.

[23j

Rivier

N.,

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91.

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J.F.,

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