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Numerical simulation of random composite dielectrics

S. Stölzle, A. Enders, G. Nimtz

To cite this version:

S. Stölzle, A. Enders, G. Nimtz. Numerical simulation of random composite dielectrics. Journal de

Physique I, EDP Sciences, 1992, 2 (4), pp.401-408. �10.1051/jp1:1992153�. �jpa-00246495�

(2)

J. Phys, I France 2

(1992)

401-408 APRIL 1992, PAGE 401

Classification Physics Abstracts

02.60 77.20 77.40

Numerical simulation of random composite dielectrics

S.

St61zle,

A. Enders and G. Nimtz

II. Physikalisches Institut der Universitit zu K61n, 5000 K61n 41, Germany

(RecHved

18 December 1991, accepted 24 December

1991)

Abstract. A novel computer simulation method is presented for the non-dissipative dielec- tric response of binary mixtures. It is based on the discretization of Maxwell's equations and thus takes into account aII classical

long-range

interactions between different particles implicitly.

The simulations performed yield a relationship between the dielectric functions of the two

com-

ponents, the volume fraction and the dielectric function of the mixture, which can be described

by an exponential formula. It was found that the exponent in this formula depends on the volume fraction but not on the dielectric properties of each component. The mixture rule is in agreement with experimental data taken from literature.

I. Introduction.

A mixture of

electrc-magnetically

diTerent materials which shows a

macroscopically

horno- geneous

behaviour,

is called "ETective Medium". For more than a century scientists and

engineers

have been

trying

to describe the effective dielectric response of such a

composite material,

for an overview see

ill.

Several theoretical

approaches

have been

developed

into formulas

characterizing

the

relationship

between the

complex

dielectric functions

(DF)

of the two components £, Em, the

respective

volume

filling

factor

(or:

volume

fraction) f

and the

resulting

effective DF ? of the mixture.

However,

there are many

approximations

necessary

in the

analyticaI deveIopment, concerning

the inner

topology

of the structures as well as

size, shape,

DF and volume fraction of the

particles.

As a consequence none of the formulas can be used to describe all

possible experimental

data.

They

are all limited to small

filling

factors

f

<

0,I) and/or

to

only

small differences between the DF'S of the components. This

problem

even occurs in the

simple

case of

water-in-oil-microemulsions,

as

reported

in [2, 3]. In this

paper we

investigate non-dissipative

dielectric mixtures

by

computer simulations and compare the results with those obtained

by

the

following

formulas:

. Maxwell-Garnett [4]

? + 2£r~

~

2£ + Em

(3)

402 JOURNAL DE PfIYSIQUE I N°4

o B6ttcher [5]

~ ~£

+ 2£m

.

Bruggeman

[6]

'-f= ~l-~~l~i)~

o

Looyenga iii

it

=

f£I

+

(I f)£I

o Lichtenecker [8]

In?=

fln£+(I- f)In£m

with Em

being

the DF of the matrix material in which

particles

with a bulk DF of £ are

randomly

distributed.

2. The method.

For the computer simulations we discretized the

3D-space

inside an ideal

rectangular cavity

resonator

using

a cubic

grid

G and a second

grid

G*

displaced

from G

by

half the

length

A of each

grid

cell in z-, y- and z-direction. The size was chosen as: 20 mm x 20 mm x 10 mm.

On the

edges

between the nodes of

G,

we define the electric field vectors and

on the

edges

of G* the

magnetic

field vectors.

Every

mesh cell of G may be filled with

a diTerent

material,

I.e.

material with diTerent

permittivity

£ or Em and

permeability

/t or /tm.

By

this

setting

~ve can

transform Maxwell's

equations

into a set of matrix

equations using

a finite diTerence method

(finite integration theory

[9]

).

By the

help

of linear

approximation

techniques for the numerical treatment of

integrals,

rot E

= -B

rot H = D

(I)

D = ££oE

B =

/t/toH

are transformed to:

C .e = -iw.b

C* h

= iw.d

(2)

D~ e = d

D~ h = b

where

D~

and D~ are

diagonal

matrices

containing permittivities

and

permeabilities

inside the diTerent cells of the

grid (as

in this work

only

materials with /t = I are studied,

D~

~vill be

(4)

N°4 NUMERICAL SIMULATION OF RANDOM COMPOSITE DIELECTRICS 403

represented by

a factor I in the

equations).

C and C* represent the discrete rot-operators [9]

and

e,d,h,b

are the discrete vectors

containing

the

respective

field

strength

of

E,

D, H and B.

Reducing

the two sets of

equations

to one we eliminate the

magnetic

field. The result is

one

single eigenvalue equation

for the electric field distribution:

C* C e =

A~£o

iLow~

Dee (3)

This discretization

approach

has the

advantage

that

continuity

conditions for the fields are

implicitly

fulfilled. Electric fields are never

computed perpendicular

to surfaces between dif- ferent materials and

magnetic

flux densities are never defined

parallel

to these surfaces. This

means that

only

the continuous components of the

electromagnetic

fields are

calculated,

a

natural property, which

always

demands some effort ifone uses finite element methods instead of finite differences.

If the resonator is now filled

only

with loss free materials

(£ real,

different

permittivities, however)

the

eigenvalue equation

is real and

symmetric (3

x N

equations

for N

nodes).

The effective

permittivity

of the mixture is then calculated from the lowest resonance fre-

quencies

of the empty

(wo)

and the filled

(w)

resonator:

~2

0

~ ~2

First we used code E of the MAFIA [9] = MAxwell's

equations

Finite

Integration Algorithm) software,

which has been

developed

for the

computation

of

eigensolutions

of such systems

by

Householder-tranformation. But the MAFIA software

package only

accepts loss free materials up to now and

we found numerical accuracy to become

inacceptably

poor for such

heteroge-

neous systems as studied here with

filling

factor

f

> 0.3.

So a new computer code COSME [10] =

Complex

Solution of Maxwell's

Equations)

was

developed

which finds the exact

eigenvalue

and

eigenvector belonging

to any resonator mode

using

a

conjugate gradient

method

together

with inverse iteration.

Consider She

general eigenvalue equation:

A~ =

qDz

First, by

a

spectral

shift

[11],

the

equation

is modified to have no

eigensolutions

with zero

as an

eigenvalue.

(A

no

D)z

= q* D ~

(4)

If no is chosen very close to the

eigenvalue

q which is

actually

to be

determined,

q*

= q no

results to be the smallest

eigenvalue

of the new

problem (Eq. 4).

Then I

/q*

is found to be the

largest eigenvalue

to the inverse matrix

(A qoD)~~D

which is

easily

found

by

a

straight

forward Mises-iteration

[11].

In the case that the inversion of this matrix is not

possible

as a cause of the

high

order of the

problem,

inverse iteration is

(5)

404 JOURNAL DE PHYSIQUE I N°4

employed:

(A

qo D ~n+i " Dzn

~n+1 ~ ~n

In each iteration step the above

equation

is solved

using

a

conjugate gradient algorithm

and

~n converges towards the

eigenvector belonging

to q* and at the same time to q, the

eigenvalue

of the

original problem (3).

In this case, the matrix A is identical with C* C and the matrix D with D~.

We obtain the effective

permittivity dividing

the

eigenvalue

of the empty resonator

by

q:

~ no

This new computer program COSME will also enable us to

investigate lossy

media in the

near future. Materials

showing dissipation

make

equation (3) complex

with a

symmetric

but non-hermitian matrix.

3. Itesults.

All the mixtures we

investigated

were

particles

in air

(or vacuum).

It can be

proved

mathe-

matically

that systems with a matrix of

higher permittivity

show the same

behaviour,

because

normalizing

all

permittivities

to the matrix

permittivity

does not

change

the

eigenvalue prob-

lem at all.

We studied mixtures

containing particles

with

permittivities

up to £ = 60. There is a

simple

reason for

choosing

this limit: the first simulations were carried out on an IBM 3084 computer

whose main memory allowed

only

40 x 10 x 40 nodes on the

grid.

As

particle

size cannot be smaller than one unit

length

A of a mesh

cell,

the smallest

particles

we simulated had a

length

d of 0.5 mm.

On the other hand it is obvious that

quasi-homogeneous properties

of a mixture can

only

be observed if the

inhomogenities

are much smaller than the

wavelength

I used for spectroscopy.

We chose the rule

~

$

~ ~~

to reduce the unwanted influence of

scattering

and reflection of the waves

by

the

particles.

The

corresponding problem

of the simulations is the

question:

how does the number of nodes in the mesh aiect the

quality

of the obtained

results,

I-e- can we be sure of

getting

rid of

finite size effects

using

a

sufficiently

fine mesh? We

compared

a very coarse mesh

(10

x 4 x 10

nodes) successively

with meshes of

increasing

fineness: 20 x 16 x

20,

40 x 30 x

40,

60 x 20 x 60, 60 x 40 x 60. The latter sizes have become

computable

because of the new vector computer in the Rechenzentrum at the

University

of

Cologne,

the NEC

SX3,

which allows

larger

systems

to be calculated

using

the program COSME. Above a mesh size of 40 x 30 x 40 the values did not

change considerably

any more. To save computer time in

general

all our models were

discretized

using

that same mesh size.

With the MAFIA programs we were able to compute the effective

permittivities

of heterostruc-

tures with a volume

filling

factor up to

f

= 0.3. Above that value accuracy was too poor to

allow a reasonable

interpretation

of the data.

(6)

N°4 NUMERICAL SIMULATION OF RANDOM COMPOSITE DIELECTRICS 405

3.5 ~

£ E

7

3 o f o-I

f 0 2

6

2.5

2.0 4

3 1.5

2

1.0

o.5 o

-10 0 lo 20 30 40 50 60 70 -lo 0 lo 20 30 40 50 60 70

E E

a) b)

14

I

12

f = 0.3

io

8

6

4

z

0

-lo 0 lo 20 30 40 50 60 70

E

c)

Fig-I-

Computer simulation data

(o)

in comparison to Maxwell- Garnett's

(i?),

Looyenga's

(o),

Bruggeman's

(m)

B6ttcher's

(b)

and Lichtenecker's

(D)

formulas, I is plotted vs, e, em = i at a

constant volume Itaction,

a)

volume fraction f

= 0.i,

b)

volume fraction f = 0.2,

c)

volume fraction f = 0.3.

First we

compared

the data

(I,e.: ?(

£,

f

with several of the effective medium formulas

(Fig.

I). Obviously

the results calculated with the formulas differ from each other and none of the formulas

reproduces

the values obtained

by

the simulation.

As

Looyenga's

formula [7]

ri/3

=

j £1/3

+

(1 f) £)3

is

clearly

the one that

gives

closest results to the numerical

data,

we chose the

generalized

mixture formula

T #

f

£~ +

(l f)

ES

to fit the data

varying

the exponent a

(0

< a <

I). Actually

for many different

tripletts

of values

f,

£,

?)

the exponents were found

using

Newton's method. An

example

result of this

procedure

(7)

406 JOURNAL DE PHYSIQUE I N°4

o.9

a

Da

f=0 3

07

t=o z

06

t=o 05

0 4

20 30 40 50 60

E

Fig.2.

= f. e° +

(I f)

e$ is used to fit the data tripletts f, e,

I),

in this case from MAFIA simulations. The resulting values for the exponent a are plotted vs. e. em

= I + I * 0.

0.8

a °

~~ .

a

o.6

o

o.5 °

o

DA

o '

o.3 ~

0.2

O-O O-1 02 03 04

f

Fig.3.

Exponent a vs. volume &action f, MAFIA

(o),

COSME (o)

is shown in

figure

2. We obtained the same exponent a out of different computer

experiments provided

that the

respective filling

factors were identical. On the other

hand,

there was

no

significant dependence

on the value of the

permittivity

of the

particles.

This behavjour

alight

reflect the interaction between the

particles becoming

stronger with

increasing

number of

particles

per unit

volume,

I-e- with

increasing filling

factor.

Figure

I

already

shows that the relative diTerence between the simulated results and the values obtained from

analytical

formulas increase with

increasing

volume fraction.

Obviously

all the formulas do not take into account the

many-particle

interaction. In

figure

3 the calculated exponent a is

plotted

us. the volume fraction. Whereas at volume fractions below 0.25 an almost

strictly

linear behaviour is

observed,

above 0.25 the linear correlation between a and

f

is abandoned.

If a

Looyenga-like

formula is

applied

to describe the

relationship

between the

permittivities

of matrix and

particles,

the volume fraction and the

resulting

eTective

permittivity

of an eTective

(8)

N°4 NUMERICAL SIMULATION OF RANDOM COMPOSITE DIELECTRICS 407

2.5 O-o

E'

. ,,

E

,

o o

o ,

2.0

.

°

i.5

lo

01 0.2

f f

a) b)

igA.

-

data

powder, from

[12]). Data calculated from

exponential formula (5): a) Real

Imaginary

part

of I.

medium, it canonly

I,e,

with an exponent a which aries with

the

filling

We compared the values iven by this formula with

the

experimental data by

Nelson

and

You [12].

From

the data shown in figure

3

we

calculated

the

a and f

as:

a( f)

=

1.65

5b)

a(f)

as

upper and ower mits for the

In figure 4 the effective ielectric unctions

of

a plastic

material

alled Kynar mixed ith air

[12]

are

ottedagainst different volume fractions in

with

the respective effective

DF'S predicted

by our

formula (5). The reement

shows

that our

simulation

data

resulting

mixture

rule are consistent with xperimental

results.

Data reported in [fl

are

also

reproduced by formula (5).

4.

nclusion.

We modeled

alculated resonance frequencies by

solving

a discretized

form

of axwell's equations. We

compared the

resulting

ffective permittivities with

the data

given by

several

analytic

mixture

ormulas.Looyenga's formula

was

found to give

the

losest values

to

the

(9)

408 JOURNAL DE PHYSIQUE I N°4

computer

simulations, although

the difference

was still very

high.

So we present a modified

exponential

formula of the form

ga(f)

=

f ~a(f)

+ j

f) ~a(f)

where the function

a(f)

may be

approximated by

a linear or a square root-like function. It describes well the data we obtained out of our computer simulations for

filling

factors below 0.3.

Generalizations to

complex

values of £

representing dissipation

are in progress.

Acknowledgements.

The

investigations

were

supported by

the Deutsche

Forschungsgemeinschaft (SFB 341)

and

by

the Bundesministerium fur

Forschung

und

Technologie /

Bonn. Discussions with D. StauTer

are also

gratefully acknowledged.

References

[1] van Beek L-K-H-,

Progress

in Dielectrics 7

(Heywood

Books, 1967) p.69.

[2] Marquardt P. and Nimtz G., Phys. Rev. B 40

(1989)

7996.

[3] Marquardt P. and Nimtz G., Phys. Rev. Lett. 57

(1986)

io36.

[4] Maxwell-Gamett J-C-, Philos. Trans. R. Sac. A203

(1904)

385.

[5] B6ttcher C-J-F-, Theory of Electric Polarization,

(Elsevier, Amsterdam,1952)

p.415.

[6] Bruggeman D-A-G-, Ann. Phys. Fr. 24

(1935)

636.

[7] Looyenga H., Physica

(Utrecht)

31

(196S)

401.

[8] Lichtenecker K., Phys. Z., XXVII

(192t)

its.

[9] Weiland T., Part. Accel. 17

(1985)

227 and 15

(1984)

245.

[10] St6Izle S., Ph. D. Th., in progress.

[ii]

Numerical Recipes, Press W-H- et al.,

(Cambridge

Univ. Press,

1986).

[12] Nelson S-O- and You T-S-, J. Phys. D, Appl. Phys. 23

(1990)

346.

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