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Ellipsometric studies of the nematic-substrate interface

J.P. Nicholson

To cite this version:

J.P. Nicholson. Ellipsometric studies of the nematic-substrate interface. Journal de Physique, 1988,

49 (12), pp.2111-2118. �10.1051/jphys:0198800490120211100�. �jpa-00210893�

(2)

Ellipsometric studies of the nematic-substrate interface

J. P. Nicholson

Dept. of Physics and Applied Physics, University of Strathclyde, Glasgow G4 ONG, Scotland, U. K.

(Requ le 16 mai 1988, révisé le 18 août, accepté le 31 août 1988)

Résumé.

2014

L’interface entre la phase nématique du 7CB et une frontière solide a été étudiée par ellipsométie optique. La différence de phase entre les rayons ordinaire et extraordinaire, 0394

=

03B4p - 03B4S, et l’angle

03C8

=

tan-1 |rp/rs| ont été mesurés en fonction de l’angle d’incidence et de la température. La modélisation des données expérimentales exige une zone de séparation exponentielle avec une densité 0,6 à 1,5 % plus grande et

un paramètre d’ordre 17 a 40 % plus grand que ceux en masse. L’épaisseur de la région interfaciale varie de 135 Å à 250 Å.

Abstract.

2014

The interface of a nematic 7CB - solid substrate has been studied by optical ellipsometry. The phase difference between 0 and E rays, 0394

=

03B4p - 03B4s, and the angle 03C8

=

tan-1 | rp/rs | are measured as a

function of incidence angle and temperature. To fit the experimental data, an exponential interfacial region having a density rising to ~ 0.6-1.5 % and an order parameter 17-40 % greater than bulk is required. The skindepth of the interfacial region varies from 135 A to 250 Å.

Classification

Physics Abstracts

61.30

-

42.80

-

68.00

1. Introduction.

There is considerable interest, both theoretical [1-6]

and experimental [7-13] in the interfacial region

between a nematic liquid crystal and its enclosing boundary wall. Apart from the well known alignment

effect of a microgrooved [18] or obliquely coated [19]

substrate which is of practical application to L. C.

electro-optic devices, there exists also an effect on

the order parameter in the vicinity of the substrate.

Thus the order parameter S (o ) at the substrate boundary is expected to differ from the bulk value

S (oo ). The functional form of S (z ) in the interfacial

region has yet to be determined, although several investigations [7-11] have been made with the nema-

tic material above its nematic/isotropic transition temperature. Measurements in this case are facili- tated by the fact that birefringence now only exists

within the interfacial region itself ; this can be

measured by obtaining the phase shift between

transmitted ordinary and extraordinary ways. How- ever, more recently total internal reflection ellip- sometry [11] has been used to investigate the iso- tropic - substrate interface, from which some knowledge of the shape of S (z ) can be inferred.

Measurements on the interface with the bulk L. C. in the nematic phase are less copious as in this

case the dominant birefringence arises from the bulk nematic phase. Semi-qualitative measurements at the nematic-substrate interface have been obtained

by Mada and Kobayashi [12] and by Salamon and Skibinski [14] who both show an enhanced order parameter near to the substrate, but obtain no

information on the skindepth of the interfacial

region. The only other work by an optical method is by this author [13] who has measured the optical reflectivity of the nematic-substrate interface. Con- siderable deviation from Fresnel reflectivity is ob-

served in the case of 7CB which leads to estimates of enhancement of the order parameter by - 15 % near

the wall and of density by -11/2 %. If a simple

linear refractive index profile is assumed, Refer-

ence 13 indicates a full skindepth of - 800 A. These results compare favourably with methods [25, 26]

which obtain S (z) from the force separating the

walls of an L. C. layer as a function of thickness.

The method used in reference 13, however is relatively insensitive to the assumed shape of S (z ). In this paper, which is essentially a continua-

tion of that work, the classical technique of ellip-

sometry [17] is used, which under certain circum- stances (e.g. varying incident angle or varying wavelength) can produce information on the index

profile of the film under investigation.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198800490120211100

(3)

2112

2. Experimental method.

The liquid crystal cell is shown in (Fig. l(a)). The

cell is filled with 7CB whilst in its isotropic phase (to

prevent flow alignment) and consists of two prisms

with their enclosing faces at a slight angle. This wedge shape enables the reflection from the upper

prism face to be selected ; the other reflection is

ignored. The upper prism is made of flint glass (Schott type F2) and has a hypotenuse microgrooved by briefly polishing unidirectionally with diamond polishing paste. The lower prism has an obliquely

coated layer of SiO such as to reinforce the planar alignment (perpendicular to the plane of Fig. 1)

caused by the microgrooving.

Prior to assembly, both prisms are subject to

intensive cleaning (the upper prism after microgroov- ing ; the lower prism prior to coating) as follows : (i) preliminary short ultrasonic cleaning (- 10 min) (ii) overnight soak in detergent (iii) several ul- trasonic rinses in distilled water (iv) several ultrason- ic rinses in 18 Mil cm deionized water. To be

pronounced satisfactory the optical surface should then be observed to drain-dry perfectly uniformly

i.e. without breaking into droplets.

Under high power microscopy the microgrooving

is seen to occupy a negligible fraction of the area of the unidirectionally polished surface. It therefore still behaves as a specular reflecting surface which is verified by the very low fraction ( 10- 7) of light

scattered off the surface. The microgrooving how-

ever, does assist in obtaining nematic alignment right through the cell (average thickness 100 J.Lm).

Uniform alignment after assembly was easily

checked by examination through crossed polarizers.

Before filling the cell with 7CB, however, the quality

of the F2 glass surface is itself investigated as

described below.

The L. C. cell is investigated for a variety of

incident angles by the apparatus shown in (Fig.1(b))

which is a conventional manual ellipsometer [17,.

The whole apparatus was enclosed in a temperature stabilised enclosure (not shown) enabling readings

to be taken throughout the nematic range. Ellip- sometry, unlike reflectometry, is sensitive to the

phase as well as the intensity of the reflected light. If rp and rS are the (complex) amplitude reflectivities

Fig. 1.

-

(a) Liquid crystal cell investigated ; n is director orientation. (b) Ellipsometer used in the measurements.

L - polarized laser ; C - 1/4 wave compensator plate ;

L.C.

-

L.C. cell shown in (a) ; A - Analyzer ; D - photodiode detector.

for the TM and TE polarizations, the respective phase shifts 8 p, 8

S

are given by :

An ellipsometer measures two quantities L1 and Q given by :

For a given incidence angle, A and Q are obtained by adjusting the incident polarization angle, P and analyzer angle, A to obtain a null response in the detector. This occurs for 4 independent values of P and A for a given compensator angle C, given by [17] :

These four null conditions were obtained for each

setting ; this not only provides a check on the reproductibility of A and Q but also leads to elimi- nation of certain systematic errors in the ellipsome-

ter, by a process known as 4-zone averaging [17] :

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We also need to correct for the effect of the side faces of the prism. Assuming each side face to be a

simple dielectric interface [20] the amplitude trans-

mittance will have no phase retardation and there- fore d is unaffected. It is easily shown that the measured Q ’ obtained from equation (4) is related

to the actual Q for the nematic substrate interface

by :

tan Q

=

cos2 (i 1- i2) tan .p’ (5)

where i1 and i2 are the angles shown in (Fig. 1(a)).

Values of A and qi were obtained as described above, firstly for the unfilled cell to obtain these parameters for the clean reflecting surface and then,

with the cell filled as described earlier with 7CB.

Quite small values of A were observed for the empty cell (~ at 40° incident angle) compared with the

values for the filled cell (differing from the Fresnel value by 20-40°). Nevertheless these empty cell

measurements were unexpectedly important as we

shall see below.

3. Analysis of results.

Typical results for two temperatures are shown in

(Fig. 2) showing the variation of A and Q with

incident angle, 60. In order to obtain information on

the variation of S and density in the interfacial

region we need to compute the reflectivities rs and rp for given refractive index profiles for both E and 0 rays. This then leads to the expected values of d

and 0 through equations (1) and (2).

The computation of the optical reflection at an

interface having a varying refractive index is a well- researched problem [15, 16, 21] having a variety of

methods some of which were summarised in our

previous paper [13]. The optical geometry chosen in this investigation (optic axis perpendicular to the plane of incidence) means that the E and 0 rays remain essentially independent of each other. In

more complicated situations the 4 x 4 matrix method of Berreman [21] would be necessary to solve the problem ; in this case we can use the 2 x 2 matrix, method described in the reviews by

Abeles [16] and Jacobsen [15]. Then optical proper- ties of the layer are described by a matrix [Mij], and

the reflectivity r is given by :

with

Fig. 2.

-

Ellipsometric data (points) and best fit curves

(for best fit case in Table I), for temperatures of 32.65 °C and 40.0 °C. (a) A

=

5 p - 5,

s

as a function of incident

angle, 00 within the upper glass prism (b) 41

=

tan-1 rplrs I as a function of 00.

Here no is the refractive index of the first medium

(F2 glass) and n2o, n2 E the ordinary and extraordi-

nary refractive indices of the bulk L. C., 00 and 02 are the ray directions in the two media respect- ively.

The matrix elements are also different in the two cases being related to the assumed refractive index

profile in the interfacial region, n10(z) in the TM

case and nl E (z ) in the TE case. Profiles (shown in Fig. 3) tried were :

Linear profile

Inverse parabolic profile

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2114

Parabolic profile

Exponential profile

Step profile

Modified Landau-de-Gennes See reference [2].

(P

=

0 or E polarization).

Here No, NE and d are adjustable parameters whilst n2o and nz E are the bulk refractive indices of 7CB [23].

Fig. 3.

-

Sketch graphs showing the functional forms tried for nlo (z ) and nl E (z), the refractive index variation in the interfacial region ; Inv. Par.

-

Inverse Parabolic ; Exp.

-

Exponential ; Lin.

-

Linear ; Par.

-

Parabolic.

In the case of the linear profile, the Mij could be

computed by the series expansion method (for d ..: A) outlined in section 3.1 of reference [13],

which was fast in computer time. The other profiles

were not analytically tractable by this method, and

were analysed by the step-matrix method in appen- dix 1, where the profile is subdivised into a large

number of small elements, each element of which

can be regarded as having a linear profile. The

accuracy of the computations were checked by comparing results with those obtained by direct integration of the EM wave equation described in

the appendix of reference [13].

4. Analysis of results.

Comparison between experimental and theoretically

calculated values of d and Q was achieved by minimizing the function M :

where yi and Ii are the experimental and theoretical values respectively (of either A and qi) for a given

00, and Ui the estimated errors.

It was found quite easy to obtain good fits to the A

data or the 1/1 data separately, especially with three

parameters (No, NE, d) available to adjust. How-

ever much more difficult is to obtain a simultaneous fit to both curves with the same parameters. To obtain such a simultaneous fit it was found necessary

to correct for the effect of the surface finish of the F2

glass substrate. Fortunately ellipsometric data had

been obtained for this surface prior to filling the cell ; this was found to be compatible with a glass

surface profile sloping linearly from the bulk value

of 1.61656 to surface value of 1.449 over a distance of 140 A, which is very similar to the results of Yokota et al. [24] on the effect on glass surfaces due

to surface leaching during polishing. The character- istic matrix [Mij] for the nematic-substrate interface is then obtained by simple multiplication [22].

where [Mglass ] is the characteristic matrix of the leached glass surface layer, and [MLC] is the matrix for the nematic interfacial region computed as

described in section 3.

With this procedure it was now found possible to

find good simultaneous fits to the Q and A data, for unique values of No, NE and d for a given profile.

Moreover the quality of the simultaneous fits shows small albeit definite preferences for some profiles

over others. Table I shows the best fit values of

No, NE, d and Mo, the (lowest) value of M for the refractive index profiles shown in (Fig. 3) and de-

fined in section 3. Apart from the results for 38.5 °C

which curiously show little preference, the trend at

all four other temperatures is a preference for a . long-tailed shape and against sharp cut-off profiles.

Thus best fits were obtain for the exponential shape, parabolic a poor second-best, linear profile an

intermediate fit, and inverse parabolic and step

profiles progressively worse fits. A profile derived

from the Landau-de-Gennes type theory of Allender

et al. [2] was also tried but the results were identical

to those for the exponential profile and are not separately listed. The theory had to be modified by allowing a density variation of the same shape as the

order parameter variation.

The results for the exponential (or modified Landau-de-Gennes) profile are shown in table II, together with those for the linear profile for compari-

son with our previous measurements [13]. This in-

cludes the surface/bulk values both for density and

order parameter which can be calculated from

No, NE, n2o and n2 E [13, 29].

Apart from the data at 32.6 °C (which may be

affected by proximity of the nematic-solid transition)

(6)

Table I.

-

Best fits to experimental data for various re fractive index profiles and temperatures

Observed tc

=

42.55 *C

the trend seems to be for d to increase steadily with temperature, and surface density and order par- ameter ratios to decrease.

Measurements were also taken above the nematic-

isotropic transition temperature but uncertainty in

the glass surface profile prevented meaningful con-

clusions being obtained. This is because in this case

the skindepth of the glass surface profile (70 A half-

width) is comparable with that of the L. C. surface

layer.

5. Discussion.

The results shown here are in qualitative agreement with our previous work [13] which indicated an unexpected large interfacial region, viz., d-

700-1 000 A assuming a linear profile. In this work for a linear profile, d ranges from 400 A up to 650 A

near the transition temperature. Thus results here,

would seem to give values of d lower by about a

factor of 0.6. However in adition to any sample to sample variations, one would expect a lower d for the present results as the previous work did not

include the effect of the initial state of the glass

substrate which, as we have seen (Sect. 4) can be represented by a surface layer having a linear profile

of thickness 140 A. This might also explain the higher surface order parameters observed in this work (11-25 % enhancement for a linear profile compared with the previous values of 9-17 % en- hancement).

Perhaps, more important, is to compare results with theory. Best fits for exponential or modified

Landau-de-Gennes profile are given in table II and range from d = 135 A at 34.2 °C to 205 A at 40.0 °C.

The theory by Allender et al. [2] predicts :

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2116

Table II.

-

Calculated values of density and order parameter enhancement from the best fit data for an exponential and linear profiles respectively. Statistical errors are random from (temperature) run to run, whilst the systematic error is due to uncertainty in the substrate surface profile and is therefore common to all runs.

and

Taking T, - T* = 1.4 °C and )

=

5 A [7]

equation (9) yields values of d ranging from

d

=

6.2 A at 32.6 °C increasing monotonically to

d

=

20.9 A at 40.0 °C. These are well over an order of magnitude less than our experimental values. The

more sophisticated mean field theory of Telo da Gama [3] unfortunately only treats the homeotropic

case. The large skindepths reported here have also been demonstrated in the case of 5CB by measuring

the force between two substrates forming a sandwich

of the liquid crystal [25, 26] reference [26] describes

both a medium-range and short range regime. In the

short range, the force oscillates over a period of

~

25 A indicating local smectic ordering which de-

cays away completely after - 100 A. The medium range force exhibits a decay of near-exponential shape having a 1/e decay distance of = 200 A.

Whilst our measurements clearly cannot detect the

short range fluctuations, they would appear to agree very closely with the medium range force distribution which is related to an order parameter variation of similar shape.

Other work which support these conclusions have been detailed in the discussion of our previous

paper [13] but it is worth mentioning again the work by Gannon and Faber [27] who infer smectic layering

at the nematic-vapour interface from surface tension measurements on 8CB and 5CB, and the X-ray

diffraction results of Leadbetter et al. [28] who infer

local smectic ordering extending over

-

150 molecules in the case of 7CB. There seems to be ample evidence therefore, that simple models

based on the Landau-de-Gennes free energy expan- sion are totally inadequate in the case of 7CB, which

has a large interfacial region

-

sometimes described

as quasi-smectic.

Our measurements in this paper are not sensitive to any smectic layering, but we can confidently point

to a strong tendency to aggregation in 7CB which leads to a higher ordered layer of - 200 A thick at the nematic-substrate interface, and which may be condensed solid phase or locally smectic in form.

The results also indicate a possible elevation of the

density near to the interface. The result at 32.6 *C for the exponential profile indicates an increase of

1.5 % - nearly twice the standard deviation of the

systematic error (due to uncertainty in the glass

surface profile). However as the temperature rises the density rise decreases and becomes barely signifi-

cant compared with the systematic error at 40 °C.

Conclusion.

The nematic substrate interface has been measured

by ellipsometry which has proved a superior tech- nique to simple reflectometry in that the method is

moderately sensitive to the refractive index profile

of the interface. Assuming an exponential profile yields a 1/e decay distance, varying from 135 A to

250 Å. Values of order parameter and density at the

surface appear to be enhanced by up to 40 % and

(8)

1.5 % respectively. A theory which includes a ten-

dency for 7CB molecules towards medium range

aggregation is necessary to explain the results.

Acknowledgments.

Thanks are due to Mr Paul Winning for making a

substantial number of preliminary measurements, and to good technical back-up by Mr. Bob Dawson.

I am also grateful for helpful correspondence from

Tom Faber (Cavendish Laboratory, University of Cambridge) and John Bunning (Trent Polytechnic), regarding the refractive indices of 7CB. Free samples

of liquid crystals are gratefully acknowledged from BDH, Poole, Dorset. As always, I acknowledge support from the Dept. of Physics and Applied Physics, University of Strathclyde.

Appendix 1.

COMPUTATION OF THE CHARACTERISTIC MATRIX BY THE

«

STEP-MATRIX METHOD

». -

The index-var-

ying layer is imagined to be subdivided into slices of width 6z each slice perpendicular to the normal (z direction) to the interface. E.M. wave propagation is

first through medium of refractive index, no, then

through the interfacial region of depth d and refrac-

tive index n (z), then finally emerging into the bulk

liquid crystal. For convenience the subscripts are omitted, but in practice the index profile n(z) is

different in the TE [nl E (z ) ] and TM [n 10 (z ) ] cases.

Consider the slice between z and z + 5z having

refractive index changing from n1 = n (z ) to

n2

=

n (z + 6z). For thin layers (Sz ’" 10 Å A ) we

can take the n variation within the slice to be linear,

furthermore we can evaluate the transfer matrix

[m ] for the slice using the series expansion method

to 1st order only [15] :

where, in the TE case :

and in the TM case

It can be shown [22] that the characteristic matrix for several layers is obtained simply by multiplying each

matrix together. Thus :

Starting with the unit matrix at z

=

0, we can now

obtain the matrix for the whole layer by successively applying equation A.4 until we reach z

=

d, the end

of the interfacial region.

For profiles with an infinite tail such as the

exponential profile or the (similar) Landau-de-Gen-

nes [2] profile, the step-evaluation needs to be taken

well beyond the skin-depth parameter, d. For the profiles examined in this paper, sufficient accuracy

was obtained by taking the evaluation out to values of z/d" 10. Unfortunately this slows up the compu- tation by the same factor. For this reason, it is advantageous to having a varying step width,

6z which becomes longer as the gradient for the profile decreases. In the exponential case this is

obtained by the simple instruction :

where 6z’ is the next step and 5z the previous. This procedure was found to speed up the computation considerably without significant loss of accuracy.

References

[1] PING SHENG, Phys. Rev. Lett. 37 (1976) 1059.

[2] ALLENDER, D. W., HENDERSON, G. L. and JOHNSON, D. L., Phys. Rev. A 24 (1981) 1086.

[3] TELO DA GAMA, M. M., Mol. Phys. 52 (1984) 611.

[4] MAUGER, A., ZRIBI, E. and MILLS, D. L., Phys.

Rev. Lett. 53 (1984) 2485.

[5] SLUCKIN, T. J. and PONIERWERSKI, A., Phys. Rev.

Lett. 55 (1985) 2907.

[6] LUCKHUST, G. R., SLUCKIN, T. J. and ZEWDIE, H. B., Mol. Phys. 59 (1986) 657.

[7] VAN SPRANG, H. A., J. Phys. France 44 (1983) 421.

[8] MIYANO, K., J. Chem. Phys. 71 (1979) 4108.

[9] BEAGLEHOLE, D., Mol. Cryst. Liq. Cryst. 89 (1982)

319.

[10] YOKOYAMA, H., KOBAYASHI, S. and KAMEI, H., App. Phys. Lett. 41 (1982) 438.

[11] HSIUNG, H., RASING, Th. and SHEN, Y. R., Phys.

Rev. Lett. 57 (1986) 3065.

[12] MADA, H. and KOBAYASHI, S., App. Phys. Lett. 35

(1979) 4.

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[13] NICHOLSON, J. P., J. Phys. France 48 (1987) 131.

[14] SALAMON, Z. and SKIBINSKI, A., Mol. Cryst. Liq.

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[15] JACOBSEN, R., Prog. Optics 5 (1965) 247.

[16] ABELES, F., Ellipsometry in the Measurement of Surfaces and Thin Films, Nat. Bureau of Stan- dards Pubn. 256.

[17] AZZAM, R. M. A. and BASHARA, N. M., Ellipsomet-

ry and Polarized Light (North-Holland, Amster- dam, 1977).

[18] COGNARD, J., Mol. Cryst. Liq. Cryst. Suppl. Ser. 1 (1982) 1.

[19] JANNING, J. L., App. Phys. Lett. 21 (1972) 173.

[20] BORN, M. and WOLF, E., Principles of Optics (Pergamon, Oxford, 1984).

[21] BERREMAN, D. W. and SCHEFFER, T. J., Phys. Rev.

Lett. 25 (1970) 577.

[22] HECHT, E., Optics (Addison-Wesley 1987).

[23] BUNNING, J. D., CRELLIN, D. A. and FABER, T. E., Liq. Cryst. 1 (1986) 37.

[24] YOKOTA, H., SAKATA, H., NISHIBORI, M. and KINOSITA, K., Surf. Sci. 16 (1969) 265.

[25] PROUST, J. E. and TER-MINASSIAN-SARAGA, L., J.

Phys. Colloq. France 40 (1979) C3-490.

[26] HORN, R. G., ISRAELACHVILI, J. N. and PEREZ, E., J. Phys. France 42 (1981) 39.

[27] GANNON, M. G. and FABER, T. E., Philos. Mag.

A 37 (1978) 117.

[28] LEADBETTER, A. J., RICHARDSON, R. M. and COL- LING, C. N., J. Phys. Colloq. France 36 (1975)

C1-37.

[29] VUKS, M. F., Opt. Spectros. 20 (1966) 361.

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