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An optical study of the interfacial region of a surface-aligned nematic liquid crystal
J.P. Nicholson
To cite this version:
J.P. Nicholson. An optical study of the interfacial region of a surface-aligned nematic liquid crystal.
Journal de Physique, 1987, 48 (1), pp.131-139. �10.1051/jphys:01987004801013100�. �jpa-00210415�
An optical study of the interfacial region
of a surface-aligned nematic liquid crystal
J. P. Nicholson
Department of Physics, University of Strathclyde, John Anderson Bldg., 107 Rottenrow, Glasgow G4 ONG,
U.K.
(Reçu le 30 juin 1986, accepté le 23 septembre 1986)
Résumé.
2014Le coefficient de réflexion optique de la zone de séparation entre la phase nématique du 7CB et une
frontière solide a été mesuré en fonction de l’angle d’incidence et de la température. Il existe une déviation considérable de la réflexion de Fresnel pour le rayon extraordinaire, mais le coefficient est semblable à celui de Fresnel pour le rayon ordinaire. La modélisation des données expérimentales exige une zone de séparation d’une
densité ~ 1 1/2 % plus grande et un paramètre d’ordre 10-20 % plus grand que celui en masse. L’épaisseur de la région interfaciale est ~ 850 A. On propose donc qu’il existe une couche quasi smectique le long de la surface.
Abstract.
2014The optical reflectivity from the interfacial region of a nematic/solid wall boundary has been measured
as a function of incident angle and temperature for 7CB. Considerable deviation from Fresnel reflectivity occurs for
the E-ray whereas reflectivities for the 0-ray are similar to Fresnel. To fit the experimental data an interfacial region having a density 2014 1 1/2 % greater than bulk as well as an increase of order parameter by 10-20 % is required. The skindepth of the region obtained is
~850 A. It is postulated that a quasi-smectic layer exists near to the boundary
wall.
Classification
Physics Abstracts
61.30
-42.80
-68.00
1. Introduction.
The alignment of a nematic liquid crystal (LC) into a single domain by the action of the enclosing cell walls
has been known since the earliest experiments [1]
where simple unidirectional rubbing was found to produce the desired results. A recent review of the various chemical and physical surface treatments has been given by Cognard [2]. The effect of the pre- treated boundary however is more complex than merely providing a uniform detector direction. In the region of
the nematic/boundary interface, the nematic molecules
experience short range forces due to the solid surface itself as well as the longer range intermolecular forces within the nematic which produce such bulk properties
as long-range order, anisotropic elasticity and viscosity,
etc. This is liable to produce localised variations of nematic parameters (such as order parameter, density, etc.) in the interfacial region from their bulk values.
Theoretical models [4-6] describing this interfacial
region have been mainly confined to temperatures
around the nematic-isotropic transition where the Land-
au de Gennes expansion [3] of the free energy in term of the order parameter, S, is valid. Their results derive
S ( z ) as a function of distance, z from the boundary ; S ( z ) is expected to decay from its value at the
boundary to the bulk value over distances of order 50- 500 A. A more ambitious approach to the problem using mean field theory to obtain the free energy in the presence of a boundary has been developed for the case
of homeotropic alignment by Telo da Gama [7] with a
further paper on the parallel alignment case expected.
Experimental measurements in the interface have been mainly confined to the isotropic phase [8-9] by obtaining the optical phase shift between light polarized parallel and perpendicular to the director after passing through the cell (parallel alignment). Measurements,
other than this paper, of the L.C./boundary interface
with the L.C. in the nematic state have been performed by Mada and Kobayashi [10], by effectively measuring
the optical transmittance of the interface, and by
Salamon [11] using fluorescence emission from a dye
loaded nematic. Both report a different order par- ameter at the surface than in the bulk but make no
estimates of the skindepth of the interfacial region.
Mada and Kobyashi’s work, in fact, is seriously marred by lack of any consideration of the effect of the
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01987004801013100
132
skindepth, d, on their results. Their expression for the optical transmission is derived using the simple Fresnel expression for the amplitude reflectivity at normal
incidence : r
=(n1 - no ) / ( nj + no ) [12] where n1 is
the refractive index of the L.C. at the boundary with
the substrate and no that of the substrate. In fact the
reflectivity of a thin interfacial layer is a complicated
function of no, nl, n2 (the bulk refractive index) and d (see below, Appendix, and Refs. [17-19]). In this paper the optical reflectivity of the interface is measured as a function of angle of incidence (not merely for normal
incidence as in Ref. [10]) ; this enables a calculation of the skindepth, d, and some indication of the profile, S ( z ) , in the interfacial region.
2. Experimental.
The cell containing the L.C. (which was heptyl- cyanobiphenyl or 7CB) and the optical arrangement
are shown in figure 1. The L.C. is contained between the hypotenuse faces of two right-angled prisms made
of F2 flint glass. The refractive index of F2 glass ( n =1.62 ) falls between the two refractive indices of
Fig. 1(a).
-Experimental arrangement for measurement of
optical reflection from glass/nematic interface. The L.C. cell is wedge-shaped to enable the reflected beam from the lower interface to be rejected.
Fig. l(b).
-Magnified view of upper glass/nematic interface showing nomenclature used. Media (0), (1) and (2) are F2 glass, L.C. interfacial region and L.C. bulk respectively.
7CB (1.65-1.68 and 1.51-1.52) thus ensuring a reason-
able reflectivity for either polarization direction. The interface is illuminated by light from a He-Ne laser at 6 328 A which may be polarized as shown in figure 1,
either with its electric field parallel to the plane of incidence, Ell (transverse magnetic or TM case) or perpendicular to the plane of incidence, El (transverse
electric or TE case). The reflected light from the first
F2 Glass/L.C. interface is detected and measured by a
Hamamatsu S1227 type photodiode followed by a
stabilized D.C. amplifier. The reflection off the lower surface emerges at a slightly different angle because the
cell is wedge-shaped, and thus can be distinguished and ignored.
Prior to assembly, the prism faces are treated to the following procedure : (i) unidirectional polishing, with
3 >m diamond paste to microgroove the surfaces in a
direction perpendicular to the plane of figure 1 ; (ii) ultrasonic cleaning in detergent ; (iii) ultrasonic
rinse in distilled water ; (iv) rinse (twice) in deionized
(18 Mfl) water. The cell was then assembled and expoxied with a 350 >m spacer at one end, to provide
the required wedge angle. Prior to filling, the surface
reflectivity was checked, to verify that it corresponded
to the expected Fresnel reflection [12] from a simple
clean surface. This confirmed that the microgrooves
were insufficiently deep or numerous to significantly
affect the reflectivity.
After filling with 7CB the cell was studied carefully
between polarizers each at 45° to the microgroove (n) direction, and illuminated by monochromatic
light. Satisfactory uniform alignment was indicated by a
uniform set of parallel interference fringe parallel to
the n direction. Each bright fringe occurs when the path
difference between 0 and E rays is an integral number
of wavelengths.
The cell was mounted on a rotating table and arranged as shown in figure la. The whole apparatus,
including laser and detector, was placed in a tempera-
ture controlled box which could be stabilized to within 0.1 °C. Reflected intensities were measured by the photodiode for varying incident angles, (J 0 as well as
over the whole nematic range of 7CB (30-42.5 °C). If V
is the actual voltage response of the detector for a given angle and Vo the response to the direct laser beam,
then the intensity reflectivity off the F2/L.C. interface is given by :
where T,
IHere, T ( i ) is the transmittance through the two
side-faces of the prism, having allowed for reflection losses. The amplitude reflectance, r ( i 1 ) , at the F2/air
faces is given simply by the Fresnel formulae [12] :
where
and subscripts ( j = 1, 2 ) refer to the first and second media (in this case air and F2 glass).
The accuracy of the reflectivity measurements
(- 2 %) was mainly limited by the stability of the
laser except at the very lowest values of R (near to
Brewster reflection) where the lower limit of the accuracy in R was ± 10- 6.
Experimental results for R are shown in figure 2
which shows the trend of R with respect to temperature
for a given incident angle, 00
=66.2°; and figures 3 and
4 which show the variation of R as a function of
00 for a given temperature.
Fig. 2.
-Experimental reflectivity as a function of temperat-
ure for constant incidence angle ( 80
=66.2° ) . Dotted lines
are the theoretical Fresnel reflectivity between glass and bulk
L.C. (i.e. d
=0). A single set of readings in the isotropic phase is also shown.
3. Theory.
An enlarged diagram at the F2 glass/nematic interface
is shown in figure 1b, giving the nomenclature used in this paper. The light is incident from the glass, which is designated medium zero, having incident angle 8a and
refractive index no. The latter is known to high
accuracy, viz. no = 1.61656 + ( t - 20 °C ) x 2.28 x
10- 6 [13]. Medium 2 is the main bulk of the liquid crystal (7CB) whose two indices, n2o, n2E, are also known from the literature [14]. Medium 1 is the inter- facial region expected to be oooooo 50-500 A thick, having
refractive indices n10 ( z ) , n1E ( z ) which become
equal to the bulk values at z oooooo d, but vary to some unknown value No, NE at the boundary (z
=0)
itself. The refractive indices are related to the local order parameter, S, by [15, 16] :
Fig. 3.
-Experimental reflectivity as a function of angle at a temperature of 32.3 °C. (a) TE polarization (b) TM polarization. The large range of values in the latter case dictated a log plot which exaggerates the similarity between
fitted and Fresnel curves.
where åa Iii is the fractional polarizability anisotropy
of the L.C. molecules and nl n 2 + 2 n2 ) /3 is the
average refractive index. A similar equation also relates the bulk values n2o, n2E to n2 and S.
Since S = S ( z ) is a function [4-7] which probably decays from a high value at the boundary to the bulk
value over the skindepth, d, both indices n10, n1E must also be functions of z, the distance from the boundary.
Therefore we have to deal with the problem of E.M.
wave propagation in an inhomogeneous or
«stratified
»medium, a subject in which fortunately the literature is
134
Fig. 4.
-As for figure 3 but at a temperature of 38.2 °C.
abundant [17-19], and which has been reviewed by
Jacobsen [17], and Abeles [18].
The optical properties of any thin film can be
represented by a
«transfer matrix
»M
=Imij] - This
relates the fields at the entrance to the film ( z
=0 ) to
those at the exit of the film ( z
=d ) by [18] :
A similar formula applies to the TM case with E and
H interchanged in the column matrices. It can be shown that the amplitude reflectivity is then given by [17] :
with
We must also use the appropriate index in medium 2 for the two cases, i.e. n2 = n2E ( TE ) and n2 = n2o ( TM ) . The matrix elements are also different in the TE and TM cases as the wave equation in the two
main cases differs (see below or Refs. [17, 18]).
To ealculate the intensity reflectivity, R = I r12, for a
given index profile n1E ( z ) (TE case) or njo ( z ) (TM case) the matrix elements mij need to be computed.
Three approaches were used, one outlined below, the others described in Appendix 1.
3.1. SERIES EXPANSION FOR SMALL WAVENUM- BERS.
-The method described here is a brief summary from reference [17]. The differential equation for both
TE and TM EM waves of amplitude U can be written
as :
with
and
for a non-magnetic medium (A ---= I-LO) , and where
nlE, o ( z ) sin 81 ( z )
=no sin 00.
For small values of k = 2 v/A, i.e. A > d, the
solutions of U can be written as a series expansion in
powers of k. The two particular solutions of interest here are F and f
=i 0, where :
For particular solutions having the required boundary
conditions (F(O) = 1; ~(0) =0; F’ ( 0 ) = 0;
¢’ ( 0 ) = ky ( 0 ) /3 ( 0 ) ), substituting in equation (7) yields:
with and
with
It can then be shown [17] that the matrix elements in
(6) are given by :
-
evaluated at z
=d.
This method was the predominant method used in the analysis since it was relatively fast in computer time. However its accuracy needed to be checked. This
was done by comparing its results for the TE case of a
linear-E profile (n E = NE ( 1 + n’ z ) which is one of
the few profiles whose wave equation solution has been
rigorously derived (Appendix 1). This comparison
showed that the series expansion method, when used to
4th power in k (i.e. v=2) gave values of R which agreed
to within 0.5 % of the rigorous solution in Appendix la
for d = 1 000 A. For d = 1 200 Å agreement fell to
-
1-2 % and then rapidly diverged as d was increased.
None of the profiles tried here was rigorously soluble
in the TM case, so TM values of R were compared with
values obtained by direct stepwise integration of the
wave equation (Appendix 2). This indicated a similar degree of accuracy in the 4th power computations for
TM reflection also.
4. Results.
,