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HAL Id: jpa-00208980

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Submitted on 1 Jan 1981

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Long-range order and diffraction of X-ray waves on multilayered crystalline films

M. Feigelman, V. Pokrovsky

To cite this version:

M. Feigelman, V. Pokrovsky. Long-range order and diffraction of X-ray waves on multilayered crys- talline films. Journal de Physique, 1981, 42 (1), pp.125-131. �10.1051/jphys:01981004201012500�.

�jpa-00208980�

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Long-range order and diffraction of X-ray waves

on multilayered crystalline films

M. Feigelman and V. Pokrovsky

L. D. Landau Institute for Theoretical Physics, U.S.S.R. Academy of Sciences, Moscow, U.S.S.R.

(Reçu le 1 S avril 1980, révisé le Il août, accepté le 12 septembre 1980)

Résumé.

2014

On calcule les facteurs de structure en diffraction des rayons X pour des films minces de smectique B.

On prédit un important effet de taille, associé à l’épaisseur du film, sur la forme non lorentzienne du facteur de structure incohérent.

Abstract.

2014

Structure factors for the coherent and diffuse scattering of X-ray waves on thin films of smectic B

are calculated. A strong size effect with respect to the width of the film as well as a non-Lorentzian form for the diffuse scattering structure factor are predicted.

Classification

Physics Abstracts

71.30

-

78.80

1. Introduction.

-

The transition from a two- dimensional crystal to a three-dimensional crystal

with an increase in the number of layers has been

studied experimentally by Moncton and Pindak in [1].

They have also studied the X-ray diffraction on thin films of a liquid crystal of butyloxybenzilidene octylanilene (40.8). The latter is smectic B in a certain temperature range. The crystal was prepared as a freely suspended film consisting of a certain number

of monomolecular layers. The number of layers varied

from 4 up to the value exceeding 100.

The problem of the development of long-range order

due to an increase in the number of layers is of theore- tical interest as well. It is acknowledged (Mermin [2], Berezinsky [3]) that a two-dimensional crystal has

no long-range configurational order. The coherent

scattering amplitude in an infinite sample equals

zero whereas the diffuse scattering amplitude has peaks at momentum transfers close to certain vectors of the reciprocal lattice. The number of such peaks

and the character of singularities are dependent on temperature (Jancovici [4], Reatto and Chester [5]h

Mikeshka and Schmidt [6], Imry and Gunther [7]).

On the other hand, in a three-dimensional crystal

the coherent scattering amplitude is different from

zero and in an ideal infinite crystal has a £5-like cha- racter whereas diffuse scattering has peaks of the

Lorentz form in the vicinity of each Bragg vector.

In the present work we investigate theoretically

how the transition from a two-dimensional to a

three-dimensional picture of diffraction takes place.

To bring the theory closer to the experimental situation, certain real features of smectic B are intro- duced into it (a small modulus of the interplane shift).

Throughout this paper the temperature regime

under consideration is assumed to be sufficiently

far from the A-B phase transition point so the influence of vortices can be neglected.

2. Scattering and fluctuations in a multilayered crystal.

-

From the very beginning it will be our

assumption that the number of layers N in the crystal

is large. The crystal will be described as a continuous elastic medium, isotropic in the plane (x, y) which corresponds to hexagonal symmetry. The elastic energy of the medium is described by the Hamilto-

nian :

Here ulk

-

components of the deformation tensor ; A., Jl, v, y and É - elastic constants ; the Greek indices a, fi acquire the values 1, 2. Expressing the Hamiltonian (1) in terms of the displacement vector Ui, we obtain :

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01981004201012500

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126

We have replaced uZ by v to stress the plane symmetry and 8 + 2 y by e. The quantities y, E are assumed to be

the same order and small in comparison with other elastic constants. This means that we regard as small all

the forces which resist the shift of the planes with respect to one another. Let us finally come to the Fourier

representation :

The finite width of the film is taken into account in (3) since the z component of the wave vector acquires a dis-

crete set of values xd

=

::!:: 2 ;n; n N

=

0, l, ..., N 2 where d-distance between the planes. From the expression

for the elastic energy (3) we may get the fluctuational averages :

Note that equations (4)-(6) are valid as for approxima-

tions in continuous media in general, only in the region of small k, K. Elsewheré k will be regarded as small, yet, the essential values of K in certain cases

appear to the order 1/d. In these cases we shall replace

the quantity x2 by its analogue for the discrete system of planes (21d’) (1 - cos Kd). In the denominator of

(4)-(6) we have neglected the quantities proportional

to e, since their contribution is always small in comL

parison with other terms.

1

Equations (5), (6) should be specified. Since y is small, the next term of the expansion over k2 should

be taken into account. Hence, instead of (5), (6) we

shall obtain

The coefficient c has the order of magnitude of Jla2

since it is physically associated with the bend of the

plane but not with the interaction between different

planes.

3. Cohérent scattering. - The cross-section for the elastic X-ray scattering off a crystal is proportional

to the formfactor S(q) equal to :

where q

-

momentum transfer, ra

-

radius-vector of a particle with the vector number a. The vector ra

can be represented in the form r.

=

a + ua. Then (7)

takes the form :

The first term of (8) corresponds to the cohérent,

and the second term to the diffuse, scattering. In this

section we shall restrict ourselves to the coherent

scattering formfactor

Let us calculate the Debye-Waller factor exp(- W ).

As is known, in the harmonic approximation

W = ’ (qu) )2. We shall be interested only in values

q equal to reciprocal lattice vectors :

where gl, g2

-

basic vectors of a hexagonal flat lattice, g3

-

vector perpendicular to the plane,

111, n, 1

-

integers. Let us first consider the case when

the vector q lies in the plane (1 = 0). In this case we

have :

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Let us separate the term with x

=

0 from the sum over K in (9), and replace the remaining sum by the integral

over K :

The first term on the right-hand side of (10) corresponds to « two-dimensional » fluctuations of the crystalline

film as a whole. With logarithmic accuracy the contribution of two-dimensional fluctuations can easily be estimat- ed as

where R - linear dimension of the system.

The quantities 1"

=

/L and fi

=

JlL where L

=

Nd - width of the film, play the role of two-dimensional Lame coefficients. At a fixed number of layers N and R - oo the Debye-Waller factor exp( - 2 W) ten4s to

zero according to the law :

The contribution of three-dimensional fluctuations to the quantity ( Ua ufl > is equal to :

At N - oo we get the Debye-Waller factor for a three-dimensional system :

In (14) we have neglected the difference of the quantity from unity. Note that the value of

exp( - Wq) for the minimum value of q is a parameter of the crystalline long-range order occurring due to the

weak interplane coupling. A similar result has been obtained by Berezinsky and Blank [7] and by Pokrovsky

and Uimin [8], for magnetic systems and by Mineev [9] for layered crystals.

In the general case when the reciprocal lattice vector q has a z-component, we add to the quantity 2 W

of (9) a term of the form

where

Note that the contribution of the mixed terms ua v* ) to the quantity W is equal to zero by virtue of symmetry.

The final expression for the Debye-Waller factor is of the form

where Y/q, wfl’ (q are defmed in (12) and (15).

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128

At 1 = 0 size effects in the Debye-Waller factor may be observed at a number of layers

For the samples of smectic B dealt with in [1] this quantity is roughly equal to 10-15. At 1 # 0 size effects in the

Debye-Waller factor may be observed at sufficiently larger N :

Under the same experimental conditions N2 is of order 300. Thus we predict a strong dimensional depenr

dence for the coherent scattering in the given regions N (cf. (17), (18)).

At sufficiently large q the coherent scattering cross-section in its maximum gets compatible with the diffuse

scattering cross-section. We can then observe only the Bragg peaks for which the following condition is fulfilled 1:

At 1 = 0 and N 11 5, the most important term on the left-hand side is the first. Therefore, the condition under

which the Bragg peaks are observed is :

At 1 :0 0 the terms involving 1 are important. Then the condition is of the form :

With an increase in N, the number of the observed peaks increases up to

4. Diffuse scattering.

-

In the vicinity of the Bragg peaks the diffuse scattering in a two-dimensional sys-

tem has singularities (cf. Introduction). Let us see what happens to them in a multilayered system. Let q lie close to any vector of the inverse lattice b. A small difference q - b will as usual be denoted as q, and the components of this vector lying in the plane of the layer and normal to it, by k and x respectively. It follows from (8) that the

diffuse scattering cross-section is proportional to the Fourier-component of the respective formfactor :

At large distances the harmonic approximation is valid :

where 4 j

=

1, 2, 3 and

The mean values of ( ui(P) uj(- p) ) have been calculated in section 2 (Eqs. (4), (5’), (6’)). Let us first treat the simplest situation when b3

=

0. The components of the correlation function Gp(r) may be calculated by the

method employed in section 3 for the Debye-Waller factor :

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where

where p and z are the components of the vector. The quantity G,(,’) should be estimated with the logarithmic

accuracy :

. 1

The contribution of three-dimensional fluctuations to the correlator G,,,P can conveniently be represented in the

form of the difference (cf. (22)). The mean values of the form ua(o) up(O) > have been calculated in (13). The

correlation function ( ua(r) up(O) > can be represented in the form

where va

=

pa/p and

(see [11], p. 741).

In the two most interesting limits we have

C-Euler constant,

These asymptotics correspond to the following behaviour of ( u,,,(r) uo(O) )(3) in various asymptotic regions :

where l5k,l-Kronecker symbol. Equation (30) has a simple physical interpretation : at small distances fluctuations of parallel displacements in various planes are independent. Therefore in each plane the correlation functions

are identical to those of a two-dimensional crystal.

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130

The behaviour of the formfactor Si(q) depends on the parameter ka , of the asymptotic form (30) of the correlation function. We get :

1, we can make use

Note that in (32) there is no dependence on K. This is natural since (32) corresponds to the region of incoherent two-dimensional fluctuations. In another asymptotic region ka fô « 1 the exponent in (21) may be considered

small, therefore the exponential function may be replaced by its argument. It actually means that the quantity Si(q) is a linear combination of the correlation functions ( u«(q) up(- q) ) :

.

where 2 W(3)

=

ba bp u.(O) up(O) )(3) is defined by (13). In (32) and (33) we have neglected slowly-changing

functions of the type k,,/N arising as a consequence of coherent two-dimensional fluctuations.

Let us now study the case when b3 components of the Bragg vector are different from zero. In this case

to the terms taken into account in the exponent of (22) should be added the following quantities :

The last term of (34) will be neglected for the time being due to its small value. Its role will be discussed below.

The correlation function for fluctuations of the transverse displacement components is calculated similarly :

The quantity ( v’(0) )(3) has been calculated in (15). The behaviour of the quantity ( v(r) v(0) )(3) in different asymptotic regions is as follows :

Let us now derive expressions for the Fourier components in différent regions of values of q. In the region ka « JYTP- applying (31), (36) and (38) we obtain :

where 0

-

angle between the vectors b and k,

(cf. [11] page 707).

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F(x)

-

gamma-function, F(a, b, c ; x)

-

hypergeometric function. Let us recall that (b - 1/y and therefore

a = 1 (b may be not small. Naturally, diffuse scattering should have singularities at certain q, there should be N

a 2. This condition coincides with the condition obtained in section 3 under which the coherent scattering peaks are observed (cf. (19b)). In (40) the term proportional to b’ corresponds to the contribution of fluctuations of the transverse displacement component v, and the remaining terms to the contribution of longitudinal compo- nents ua. Note the different power laws followed by the asymptotes of Si(q) depending upon the relations yk2/vx2

or YK lyk .

In another asymptotic region ka » JYTP, at bl! # 0 applying (30), (36), (39) we get :

The dependence on x in this case cannot be observed due to the ô-like character of the correlation function ua(r) up(O) )(3) (cf. (30)). At b ~ = 0 the dependence on K is :

Let us now study the previously neglected contribution of the mixed fluctuations ui(q) v(- q) ) to Si(q). Fluc-

tuations of this type lead to the appearance in Si(q) of the term involving the first harmonics in the angular depen-

dence in the plane k : 8S;(q) (kb~). In particular, in the region ka » y/, applying (6’), (30), (36), (39) we get :

In conclusion, note that the weak interplanar interaction leads to two effects. The first of them, comparati- vely obvious, is the increase of the diffuse scattering background which has been mentioned in [1]. The second

is the non-Lorentzian (power-like) form of the diffuse scattering peaks at non-zero values of b3 (cf. (40». The possibility for observing such peaks comes about because the exponent a

=

(b/N determining the deviation of

the line from the Lorentzian line may be not small at N » 1 since (b - 1/y.

References [1] MONCTON, D. E., PINDAK, R., Preprint, Bell Lab., 1979.

[2] MERMIN, N., WAGNER, H., Phys. Rev. Lett. 17 (1966) 1133.

[3] BEREZINSKY, V. L., ZhETF 59 (1970) 907.

[4] JANCOVICI, B., Phys. Rev. Lett. 19 (1967) 20.

[5] REATTO, L., CHESTER, C. V., Phys. Rev. 155 (1967) 88.

[6] MIKESHKA, H. J., SCHMIDT, H., J. Low Temp. Phys. 2 (1970) 371.

[7] IMRY, Y., GUNTHER, L., Phys. Rev. B 3 (1971) 3939.

[8] BEREZINSKY, V. L., BLANK, A. Ya., ZhETF 64 (1973) 725.

[9] POKROVSKY, V. L., UIMIN, G. V., ZhETF 65 (1973) 1691.

[10] MINEEV, V. P., ZhETF 67 (1974) 1894.

[11] GRADSHTEIN, I. S., RYZHIK, I. M., Tables of integrals, sums,

products, Moscow 1971.

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