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HAL Id: jpa-00208649

https://hal.archives-ouvertes.fr/jpa-00208649

Submitted on 1 Jan 1977

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Classical electrodynamics of non-specular conducting surfaces

F. Flores, F. García-Moliner

To cite this version:

F. Flores, F. García-Moliner. Classical electrodynamics of non-specular conducting surfaces. Journal

de Physique, 1977, 38 (7), pp.863-870. �10.1051/jphys:01977003807086300�. �jpa-00208649�

(2)

CLASSICAL ELECTRODYNAMICS OF NON-SPECULAR CONDUCTING SURFACES

F. FLORES and F.

GARCÍA-MOLINER

Instituto de Fisica del Estado Sólido

(CSIC

and

UAM),

Universidad

Autónoma, Cantoblanco,

Madrid

34, Spain

(Reçu

le 15 décembre

1976,

révisé le 14 mars

1977, accepté

le 18 mars

1977)

Résumé. 2014 Pour les milieux conducteurs dispersifs le rôle de la diffusion

superficielle

d’électrons est étudié dans une approximation semi-classique en utilisant un paramètre spéculaire phénomé-

nologique p

(0 p 1). Le problème de l’accumulation de charges non physiques sur la surface, qui apparait souvent dans les

développements

en p, est

explicitement

discute et évité. La relation de

dispersion

du

plasmon

de surface de mode-P dans la limite

quasi-statique

(c ~ ~) est obtenue pour p et 03BA (vecteur de propagation) arbitraires. Ceci permet une étude de l’effet de diffusion sur l’atténuation du

plasmon

de surface et aussi des différents rôles des fonctions

diélectriques longitudinales

et

transversales. Ceci est illustré par

l’application

d’une formule

d’interpolation simple

pour les fonc-

tions

diélectriques.

Abstract. 2014 For

dispersive conducting

media the role of surface scattering of electrons is studied in a semiclassical

approximation

using a

phenomenological

specularity parameter p (0 ~ p ~ 1).

The problem of

unphysical charge

accumulation at the surface, which often appears in treatments in terms

of p,

is

explicitly

discussed and avoided. The P-mode surface

plasmon dispersion

relation in the

quasistatic

limit (c ~ oo) is obtained for

arbitrary

p and 03BA

(propagation

vector). This

permits

a study of the effect of surface

scattering

on surface plasmon

damping

and also of the different roles of the

longitudinal

and transverse dielectric functions. This is illustrated with an

application

in terms

of

simple interpolation

formulae for the dielectric functions.

Classification

Physics Abstracts

8.170

1. Introduction. - This paper follows a

previous publication

- henceforth denoted as

[1]

- which

discussed the

general problems

of

electromagnetic matching

at the surface of a

dispersive

non

conducting

medium. The case

of dispersive

conductors will be discussed

here, concentrating

on the surface

plasmon dispersion

relation

(S.P.D.R.)

in the

quasistatic

limit c - oo. The idea is to

investigate

the effect of ’ surface

scattering

for non

specular

surfaces. It is well known that the

theory

of surface

plasmons

in metals

needs to be extended

beyond

the semiclassical

approxi-

mation.

Quantum

mechanical interference effects between incident and reflected electronic wavefunc- tions and details of the surface

potential

barrier are

very

important.

While all this is

commonplace

in

current literature on the

subject,

the effect of surface

scattering

has been studied much less. A serious

investigation

of surface

scattering

within the semi- classical

approximations

was undertaken

by

Zaremba

[1] using

a Boltzmann-Vlasov

approach

and

all the structure of the dielectric function of the electron gas which is contained in the random

phase approximation. Explicit

results were obtained for the

long

wave limit on the basis of detailed numerical

computations

carried out for different

assumptions

about surface

scattering,

in

particular

for the

specular

and diffuse cases. Zaremba

[1]

very

appropriately

stressed that diffuse

scattering

must be treated with

care. There must be some way in which the

incoming

current - here denoted

by J - reaching

the surface must return into the bulk.

It is customary to use a

phenomenological

model to

describe surface

scattering

in terms of a parameter p which can take values between 0 and 1 and is

something

like the total fraction of

specularly

reflected electrons.

Of course this

description glosses

over the actual

problem

of the detailed

probability

of

scattering

of an

incoming

state k into and

out-going

state

k’,

but for the time

being

it seems to be very difficult to go

beyond

this model and still have a

fairly

flexible method to

perform

a

physical analysis ending

in

practical

calculations. For the

S.P.D.R.,

which is the concern

of this paper, Zaremba’s

[1]

work is the most articulate attempt at

studying

the effect of surface

scattering, taking

care to avoid the accumulation of

charge

at the

surface.

Precisely

for this reason the formulation in

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01977003807086300

(3)

864

terms of the parameter p was

rejected

and different

assumptions

about surface

scattering probability

were made

separately.

These consist in

assuming

different forms of

angular dependence.

Between the extreme cases of

specular

and

completely

diffuse

scattering

two

plausible specific

forms were

assumed,

in some way

representing

intermediate situations.

Thus, although

these calculations bear out the effect of surface

scattering, they

are not calculations from first

principles

and

ultimately

amount to different

phenomenological

models. It would seem desirable to have a solution in terms of the

phenomenological

parameter p which can then be varied

continuously

or even treated as an

adjustable

parameter. It is also

clearly

desirable to have a solution to the

problem

for

arbitrary

wavevector K

parallel

to the surface.

This will be the purpose of this paper and will also be

a natural continuation of the

investigation

undertaken

in

[I].

It is of value to

recapitulate briefly

the

approach

to the

problem. (i)

Given the medium in z > 0 and the

vacuum in z

0,

a

hypothetical

extended medium

(M)

is defined and likewise a

hypothetical

extended

vacuum

(V). (ii)

The definition of

(M)

includes

fictitious - surface and volume - stimuli and has a

field

Tm everywhere.

Likewise for

Tv. (iii)

The real

system is reconstituted

by matching

the real

(p(zO) = (pv(zO)

to the real

(p(z>O) = qJM(Z>O).

This

provides

the

matching

or secular

equation.

(iv)

The model is

prescribed by imposing

a definite

relationship

between

q>M(Z 0)

and

q>M(Z 0).

This

provides

the

subsidiary equations

necessary to elimi- nate the

parameters

introduced in the definition of the fictitious stimuli.

It is

important

to stress that

simply taking

the

limit c -+ oo in the results of

[I]

would be incorrect for conductors. The reason is the

problem

of

charge

accumulation’

just

discussed. This is most

clearly

seen

by considering

the electron distribution function

f (r,

v,

t),

which can be written as :

f i being

the correction to the

equilibrium

distribution

fo(v).

In standard treatments

fl(r,

v,

t)

is determined

as a function of the electric field E

by solving

the

linearized Boltzmann

equation,

with some

boundary

conditions. Here we are concerned with the surface condition on

11 (r,

v,

t).

In the usual way

[3]

this

condition states that a

fraction p

of the incident electrons are reflected

specularly,

while the rest

undergo

diffuse

scattering.

This

implies

where

6fi

represents the distribution for electrons

scattering diffusely.

Notice that we cannot write

bfi

=

0,

since this would

imply

that a fraction

(l-p)

of electrons is

disappearing

in the surface instead of

being diffusely

scattered. Similar considerations are

made in

[1, 2]. Moreover, bfl

must have such a value

that the total

perpendicular

component of the current

density

is zero at the surface z = + 0.

However,

this is a condition

determining

a scale factor but not the form of the distribution function

bfl

itself. Different authors have

postulated

different forms of

bfl.

For

instance,

Keller et al.

[2]

have

proposed

A

being

oc

exp[i(K.p - rot)],

where k =

(K, A)

and

r -

[p, z] ;

while Zaremba has used other alternatives such as

or

0

being

the

angle

between v and the normal to the surface. These last distribution functions are

reflecting

a certain

degree

of surface

anisotropy

as Greene’s

work

suggests [4].

Here we have taken

bf as :

This choice allows us to

simplify

the

problem

asso-

ciated with the surface

boundary condition,

since in this way the condition on the distribution function

can be simulated

by

a surface electric field. The idea is to use an extended

medium,

and substitute the

boundary

condition at the surface z = + 0

by

a

properly adjusted

electric field zo

E+ b(z) ei(K.p-rot).

In this case it is an easy matter to find the

perturbed

distribution

function, by using

a formulation

[5]

equivalent

to the Chambers method

[6],

in which

the

perturbed

distribution function is

given by

where a past local time t’ for the electrons is introduced

by using

the

path

variable method

[6] (e

is the electron

charge).

It can be

readily

seen that

introducing

a

6-function field - as indicated above - into this formula

by

itself

produces

a distribution

(4)

This

expression

bears out the cos 0 factor and shows how this form for

bfl

results from a fictitious electric field normal to the surface. This trick will be used later to obtain a zero current

density

at the

surface, by conveniently adjusting

a surface electric field in the fictitious extended medium. In order to understand this

point clearly

it is

interesting

to

analyse

in detail

the structure of different types of surface stimuli.

This will be done

in §

2.

2.

Symmetric

and

antisymmetric

surface stimuli. - The wavevector will

always

be of the form k =

(K, 0, A),

where A will be

ultimately integrated

away and x will be the

propagation

vector

parallel

to the surface. The

symmetric

case is trivial. One

puts

a surface stimulus of the form

uM(K, (0) b(Z), i.e.,

in Fourier

transform, e(K, W)

=

e. Then,

for an

isotropic

medium

[I]

from

and the

divergence equation

the scalar

potential

in the extended

hypothetical

system

(M)

is

given

in Fourier transform

by

This

generates

a field with mirror symmetry. Hence- forth the

explicit dependence

on

arguments

such as r,

k,

etc., will

only

be indicated whenever necessary.

Likewise for the extended vacuum

(V)

In the real

system Dz

must be

continuous, i.e.,

Ð;( - 0) = Dt(+ 0),

or, with

t? = ! I z I 0,

whence

a’ = - a.

All the

integrations

are under-

stood from - oo to +00. The

dispersion

relation

(S.P.D.R.)

follows from the

continuity

of cp in the real system,

i.e., T’(- 0) = Tl(+ 0),

whence

a well known solution for the

specular

surface

model

[7].

This is also the limit c - oo of the result obtained in

[I],

and

corresponds

to the case p = 1.

It is also

interesting

to discuss the

antisymmetric

case p = -

1, although

we stress that this is an

unphysical example

for conductors since p,

being

a

real

fraction,

takes

only

real values in the interval

(0,1 ).

However,

this case is discussed here because the formalism thus

developed

will be used later as

part

of the method

employed

to obtain a

physically

valid

solution for

arbitrary

values

of p.

An

antisymmetric

field can be obtained much in the

same way as

explained

in

[I].

Since in this case

E( - 0) = Et( + 0),

and.

EM( - 0) = - Et( + 0),

one can write :

This

signifies

a fictitious surface stimulus of the nature of a

magnetic

current

creating

an

antisymmetric

field.

We stress that eqs.

(4)

reduce to

O. DM

=

VAEM

=

0,

for z >

0,

the electrostatic

equations

for the real

system,

for all z > 0. In other

words,

when we extend the medium in z > 0 to the whole space, we can

extend

similarly

the electrostatic

equations,

with the

sole constraint that the extended

equations

agree with the real ones for z > 0.

Now, taking tt

in

the y

direction and

integrating

the curl

equation

DM

is now

purely

transverse :

whence

Hence there exists a vector

"’M

=

(0, tf¡M, 0)

such that

Then

whence,

from

(4),

and,

in Fourier

transform,

For later reference :

Equations (5)

and

(6) with ET

= 1 describe

(V) and,

as

usual,

since in the real system, at z =

0,

(5)

866

it follows that

whence jV = - jM,

which used in the condition

yields

the S.P.D.R.

This is different from

(3),

since it

corresponds

to a

different -

unphysical

- model. It is also the limit

c - oo of the result obtained in

[I]

for p = - 1.

However the

point

to notice is that this

provides

an

antisymmetric

field

but,

as can be seen from the fields

given by

eqs.

(6),

the real electric current thus cons-

tructed fails to

satisfy

the condition

j_,(+ 0)

= 0. In

order to achieve this it is necessary to invoke another

antisymmetric

field. This other

antisymmetric

field

can be built up

by using

a surface

dipole, i.e.,

a surface

charge

which is

proportional

not to

b(z)

but to its

derivative. In this way, instead of eqs.

(4)

we have the

following

extended

equations :

The

corresponding antisymmetric

scalar

potential

is

where

ÐM

= 4

n’J)M(K, w),

and likewise for

(p’

with

’6L = L Notice that an

antisymmetric

model is

being

constructed but now the response is

governed by EL

instead of GT.

Now,

the scalar

potential (8) gives

the

fields EM and DM. In

particular

and also

From the

continuity

of

D,,

in the real

system, 5)v = 9)m

and from the

continuity

of T in the real

system,

This

dispersion

relation is different from

(3)

and also

from

(7). Furthermore,

this field also

yieldsj,(+ 0):o 0.

We can now see how one could build up a formal

solutions

for the case p = -

1, satisfying

the condition

jz( + 0)

=

0, by

a proper combination of the two

previous antisymmetric

cases. In order to achieve

this,

let us discuss a

peculiarity

of the fields

given by

eqs.

(9).

The field

D’

can be rewritten as

The constant term

Om

in

DI(A, z) gives

a ð-function

in real space,

i.e.,

a

singularity

in the z

component

of

Dm

for the second

antisymmetric

field. This

singularity

appears

equally

in EM

giving

a contribution to the

perturbed

distribution function of the form discussed

in §

1. This source

gives

rise to a contribution to the normal current

jz(+ 0),

which can be used to account

for all the backflow of

charge

which would otherwise be lost in the

diffusely

scattered fraction.

It follows from this that the formal construction of the

antisymmetric

extended medium

(M)

would

require

a combination of the two

antisymmetric

cases,

where the surface

dipole

and the surface electric field

are

adjusted

in order to achieve

j,, .(+ 0)

= 0. This

would

yield

a

formally

valid solution for p = 2013 1

which, however,

is of no

physical

interest and will not be discussed any further.

Instead,

we shall

proceed directly

to construct the

complete

solution for the

case

0 p 1.

It is now clear that the construction of the extended medium

(M)

for a

general

model of surface

scattering requires

a combination of three types of fictitious

stimuli, corresponding

to the

symmetric

and to the

two

antisymmetric possibilities,

the last two

having

different roles and

involving

different parameters.

It is rather cumbersome to have to treat the two

antisymmetric

terms on a different

footing,

as describ-

ed in

(4)

and

(8),

but this can be

easily

avoided

by

means of a formal device as follows.

Consider the electric field

EM obeying (4).

Its curl is

zero

everywhere

except at z = 0.

Thus,

there exists

some scalar

potential rp’

such that E’ = -

V(p’

is the

same as

EM

of

(4)

for all z =A 0. The two terms will

only

differ in a

possible

6-function

singularity

at z = 0.

In Fourier

transform,

This will have the same behaviour as EM of

(8)

if

T’

is

chosen to have the form

Then

This field will therefore be

equal

to the first

antisymme-

tric field

EM obeying (4), making

the identification

(6)

aK

= jM

and

remembering

that the

singularity

at the

origin, corresponding

to the

Â.-independent

term

in

(11),

must be removed when

writing

down the

field

in real space. With this device all terms

contributing

to the field in

(M)

can be described on the same

footing,

which makes the

analysis

a great deal

simpler.

3. Surface

plasmon

relation for

arbitrary

p. - After the discussion

in § 2,

the extended system

(M)

is

defined to have the

following

field

We stress that the first and third terms,

although formally similar,

are

going

in fact to

play

different

roles.

The first term is

antisymmetric.

Notice that the dielectric function of the medium does not appear in this term. Its role is to

provide

the

appropriate

functional

dependence

on A to

give

an

antisymmetric

field. The 6-function

singularity

must be removed

before writing

down the

corresponding field

in real space.

In

practice

this is achieved

by making

the substitution

before integrating

over ,1,. The second term is the

symmetric

one. Since its

À.-dependence

is

different,

so

is its

z-dependence

in real space. Thus with the surface stimulus

uM(K)

alone a fixed

relationship

between

(P’(z 0)

and

cpM(Z

>

0)

cannot be achieved for all z. For this reason it is necessary to add a bulk

charge

distribution measured

by f

=

f(", A). However,

since

T’(z

>

0)

must be

equal

to

T(z

>

0)

for the

real system,

f

must not

give

rise to any bulk

charge

for z >

0, i.e.,

must not have

poles

in the’ upper

half plane-complex

,1,

plane.

The last term is the response of

(W

to a surface

dipole stimulus,

as discussed

in §

2.

It is also

antisymmetric

and of course this surface stimulus must be screened with EL. The role of this term is to

produce

the surface source to ensure

conservation of

J,.

As for

(V),

it suffices to use

The programme can now be carried out as follows.

The S.P.D.R. is obtained in

general

form from the conditions that in the real system cp must be continuous

at z = 0, i.e.

and likewise for

Dz.

The first condition can be written down at once. Thus

The second condition

requires

some care, in

particular,

the substitution indicated in

(13)

must be made in the

D,,

component derived from the first term of

lpM

in

(12).

This

yields

Introducing

the parameters

equations (14)

and

(15) yield

the

general

form of the S.P.D.R.

The term in X2 is the new-source-term which would be absent from the limit c - oo of the results obtained in

[I].

The task now is to find xl, X2

and f

This comes from the

following

conditions :

(i)

The definition of the model in

terms of p, i.e.,

(7)

868

(ii)

The

requirement

that the

net Jz

must be zero at z =

+ 0, i.e.,

These conditions can be written down

knowing qJM

from

(12)

and hence E’ and

DM.

The result

depends

on

integrals involving EL

and ET. At this

stage

the

following

model will be

chosen,

with

and

with

Then,

in

evaluating

terms like

there are two contributions. One comes from the

pole

at A = ix and

gives

a term in

exp( - xz). The

other one

comes from A = iL and

gives

a term in

exp( - Lz). By itself, f gives

no extra contribution since it has no

poles

in the upper half

plane. Thus,

on

closing

the

integration

contours in the lower half circle at

infinity,

the A

depen-

dence of

f

must not leave a residue of its own, so that the same two

exponentials

appear for z 0. This is satisfied for a functional

dependence

of the form

Then, imposing

the condition

(18)

for the two

exponential

functions

of I z separately yields

the two

subsidiary equations

and

where E =

E(k

=

0, w)

= 1 -

cv§/cv.

For condition

(19), Ez

and

Dz

must be derived

again

from

cpM

in

(12) remembering

the substitution

(13)

for

the contribution of the first term. This

yields

The three fictitious parameters are eliminated

by using

the three

subsidiary

conditions

(24), (25)

and

(26).

It is

trivially

easy to rewrite these as a set of three

inhomogeneous,

linear

algebraic equations

for the unknowns xl,

X29 B

and to see that the

inhomogeneous

term is

proportional

to

(1 - p).

The determinant of the coefficients is

always 0 0,

for

arbitrary

x

and p,

and in

particular for p

= 1.

Thus,

xl = x2 = B = 0

for p

= 1.

Using

this in

(17) yields again

the trivial result

(7)

for the

purely specular

model.

(8)

For

arbitrary

p, the values of x 19 X2 and B obtained from

(24), (25)

and

(26)

are to be used in

(17) which,

for

these model dielectric

functions, yields

the

following explicit

result for the S.P.D.R. :

valid for

arbitrary K and p.

This result is

significantly

different from the limit c - oo of the result of

[I],

due

to the source term in X2-

The S.P.D.R.

for p :0

1 has been studied

by Quinn [8]

for small values of

(1 - p), i.e.,

for

nearly specular surfaces,

as a power series in

(1 - p).

Unfortunately

no

comparison

with the

present

results

can be made because the

analysis

made no

provision

for conservation of

J.

As indicated

in § 1,

Zaremba’s

[11

work does conserve

J,.

Since

explicit

results were

given only

for the

long

wave

limit,

this

limit will be studied

in §

4.

4. The

long

wave limit. -

By studying

the

disper-

sion relation

given

in

(27)

it is seen that ii this is written

so that the factor

(2 QJ2 - (02)

is isolated on the

I.h.s.,

then the

following practical

rule must be

observed for all the terms

appearing

on the r.h.s. : Put 8 =

1,

co =

(t)p/,/2-,

evaluate

B, l,

L and t to

lowest order -

i.e.,

for x = 0 - and xi to

first

order

in K. Care

must be exercised for

10

and to, since

J-=t

can be ± i. The correct results are

and,

to lowest

order,

while to first order

This

yields

the

long

wave S.P.D.R.

The next

question

is the choice of

PL

and

PT.

The

forms used

for 8L and &r

can be obtained from the

complete

formulae of Lindhard

[6] taking VF k

fixed

and

considering

the lhnits cv « Up k and CO >> VF k.

This suggests

for 8L

and &r

interpolation

formulae of the form of

(20)

and

(22)

with

PL

= VF

,,/3-/,/5-

and

PT

=

VF/J 5. Then,

with úJo =

úJp/j2, (28)

can be

written in the form

where

The real

part

does not

depend

on p. This is an

artifact of the

simple

model used for dielectric func- tions.

However,

it is

interesting

to compare with the far more elaborate

computations

of Zaremba

[1]

who used the full R.P.A. We recall

from §

1 that our

model of surface

scattering

is

specular

when p = 1 and

corresponds

to Zaremba’s cos 0

scattering

model

when p = 0. Thus our result

(29)

must be

compared

with these two cases. Zaremba’s actual results are

C = 0.394 - i 0.002 1 for the

specular

model and

C = 0.362 - i 0.131 for the cos 0 model. It is gra-

tifying

to see that rather similar

figures

are obtained

in the present

simplified analysis

which is based on

very

simple

dielectric functions and can be carried

through

in

analytic form,

not

only

for

long

waves, but also for

arbitrary K

and p.

5. Conclusions. - In the

spirit

of

[I],

this paper shows that it is not necessary to invoke additional

boundary

conditions in order to solve the

problem

of surface

matching

in the classical

electrodynamics

of

dispersive

media. The

proof

consists in

giving

the

explicit

solution - in this case for the S.P.D.R. -

by proceeding directly

from a

physical model,

here

described in terms of the surface

scattering

parame- ter p.

Although

the form of the dielectric functions for reasonable models may be the same, the case of conductors is

physically

different from the ’ case of dielectrics or excitonic

systems

in

that p

takes real

values in the interval

(0, 1)

and in that for all values except p = 1 one must face the

problem

of current

conservation in the direction

perpendicular

to the

surface. For this reason the results of

[fl

cannot be

simply

extended

by letting

c - oo. It has been

necessary to redo the

analysis including

a surface

source term to cancel out the artificial sink of

charge

which would otherwise be hidden in the formalism.

This is not a trivial matter. It is instructive to see

what one would obtain without the source term.

In this case the

dispersion

relation has still the form

(9)

870

of

(27),

but X2 is now zero and x, and B are different.

The result for IOW K is then

For all

but p

= 1 this differs

significantly

from the

correct result

(28).

In

particular,

this would lead to the

erroneous conclusion that one has found a

dependence

of the real

part

of cv on the model for surface

scattering.

Of course, there is a small

dependence,

as evidenced in

a more accurate

computation using

the full structure

of the dielectric function

[1].

This difference is a small order effect which is missed out in a crude estimate such as the

present

one based on the

simple interpo-

lation formulae

(20), (22).

The

origin

of the difference

between

(28)

and

(30)

is

physically interesting

in

itself. In the random

phase approximation

one can

show

[9]

that the coefficient of K is

proportional

to the

dipole

moment of the

charge density

fluctuation associated with the surface wave. It has been further shown

[10]

that this holds on

general grounds, irrespec-

tive of the

model,

if one does not take account of surface

scattering.

More

generally

one finds

[10]

the

dipole

term and also another term

associated

with the current

density

fluctuations

parallel

to the surface.

More will be said

presently

about this extra term, which is

mainly responsible

for the

damping

contained

in the

imaginary

part.

Now, looking only

at the real

part in

(28)

and

(30)

it is clear

why they

differ. An incorrect

charge

sink is

responsible

for a false des-

cription

of the

dipole

moment in the

region

of the

surface wave. For p = 0 this reduces Re C in

(30)

to

one half of its correct value. The smaller difference between

(28)

and Zaremba’s

[1]

more accurate result

is due to the same reason. The

charge

densities - and

hence their

dipole

moment -

differ, although

not too

much,

because different dielectric functions are

being

used. One could

always

carry

through

the present

analysis

with a more elaborate dielectric

function,

but this is outside the scope of this paper, which aims rather at

having

an overview of the

problem.

It is

more instructive to

study

the effects of

spatial

dis-

persion by looking

at the

imaginary part

for

which,

as stressed elsewhere

[10],

the effect of surface scatter-

ing

on the current

density

fluctuations is

mainly responsible.

It is seen in

(29)

that this is zero for

p =

1,

and is of the same order as Zaremba’s result

[1]

for the case

corresponding

top = 0. Indeed Zaremba’s result for

specular

surface

scattering

-

corresponding

to p = 1 in

(29)

- is an order of

magnitude

smaller.

Bearing

in mind that the model used in all cases is collisionless in the

ordinary

sense, the

meaning

of these

results is

quite

clear. Of course the smaller order contribution is the effect of Landau

damping,

which

again

is missed out when the

interpolation

for-

mulae

(20), (22)

are used. The main effect comes from

the lack of surface

specularity,

which introduces a loss of momentum

parallel

to the surface.

Again

it is seen

that an

approximate interpolation

formula

for h

can

produce

the main contribution to this term.

The essential

point

is that it is

dispersive.

If one uses

instead a local dielectric function 8 = 1 -

w;1 W2

one obtains - i

0.023(1 - p)

tor Im

C, i.e.,

an

order

°

of

magnitude

smaller than the value obtained from a

simplified dispersive

function

ET(k, w).

The lesson

, from this

simple

exercise is that the current

density

fluctuation term is very

important

for the

decay

of

long

wave surface

plasmons

and that it

images

rather

conspicuously

the effects of

spatial dispersion

of the

medium.

This paper for conductors

together

with the one

previous [fl

for dielectrics

give

a

complete

solution to

the classical

electrodynamics

of the surfaces of

dispersive

media valid in the classical

approximation.

We have

actually

discussed here

only

the

quasistatic

limit because this is in

practice

most often the case of

interest when

studying

surface

plasmons

in metals.

Work is now in progress on the extension of this method to include retardation effects in order to

study reflectivity

and related

electrodynamical

pro- blems in metals.

Our

analysis

focuses on the effect of the surface as

described in terms of the parameter p, which allows for a

plausible phenomenological

model of surface

scattering.

Further necessary

improvements

of the

theory require going beyond

the semiclassical

approxi-

mation and

beyond

the

simplest

barrier models for the surface electronic

potential.

For the electron gas these

problems

are the

subject

of a

great

deal of current

activity,

without however

incorporating

an

explicit study

of the effects of surface

scattering.

The present work is in this sense

complementary.

It is

hoped

to

undertake a further

investigation

in which the ideas

expounded

here can be

incorporated

in a more

advanced scheme.

References [I] GARCÍA-MOLINER, F. and FLORES, F., J. Physique 38 (1977).

[1] ZAREMBA, E., Phys. Rev. B 9 (1974) 1277.

[2] KELLER, J. M., FUCHS, R. and KLIEVER, K. L., Phys. Rev. B

12 (1975) 2012.

[3] MAXWELL, J. C., in The scientific papers of James Clark Maxwell, W. D. Niven (Ed.) Dover, N.Y., 1965, p. 703.

[4] GREENE, R. F., Crit. Rev. Solid State Sci. 4 (1974) 477.

[5] FLORES, F., GARCÍA-MOLINER, F. and NAVASCUES, G., Surf.

Sci. 24 (1971) 61 ;

FLORES, F. and NAVASCUES, G., Surf. Sci. 34 (1973) 773.

[6] CHAMBERS, R. G., in The physics of metals. I : Electrons, J. M. Ziman (Ed.) (Cambridge University Press) 1969.

[7] RITCHIE, R. H. and MARUSAK, A. L., Surf. Sci. 4 (1966) 995.

[8] QUINN, J. J., Solid State Commun. 11 (1972) 995.

[9] HARRIS, J. and GRIFFIN, A., Can. J. Phys. 48 (1970) 2592.

[10] FLORES, F. and GARCÍA-MOLINER, F., Solid State Commun.

11 (1972) 1295.

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