2
18
M.K. Sanyal et al. / Physica B 248 (1998) 217—222
monolayer, and, in general, the actual mechanism
of salt formation during the transfer of the mono-
layer to the substrate is not clear so far. However, if
an LB film is deposited from a monolayer of
a preformed salt of a fatty acid, such as ferric
stearate (FeSt) on water, at least the uncertainty in
the monolayer composition is much reduced.
Our understanding regarding the nature of cor-
relation in the interfaces [8] and the nature of
molecular stack [9] in these films are also far from
complete. The stability of the interfaces present in
these films are intriguing, too. It was shown re-
cently that by exposing a cadmium arachidate
ly alkaline (pHK8.0). Fourier transform infra red
spectra of the purified bulk FeSt sample, as well as
a 11 ML LB film of this FeSt on calcium fluoride,
could not detect the presence of hydroxy fatty acid
salts. A 9 ML LB film of this preformed and purifi-
ed FeSt was deposited on a Si(1 0 0) substrate at a
surface pressure, temperature and subphase (water)
pH of 30 mN m\ꢂ (surface tension 42 mN m\ꢂ),
25°C and 5.6, respectively. The deposition rate was
3 mm/min. Details of the sample preparation, puri-
fication and LB deposition have been provided
elsewhere [12].
(
CdA) LB film in an hydrogen sulphide (H S) envi-
ꢀ
ronment, cadmium sulphide (CdS) nanostructures
can be formed [10] without much disturbance to
the embedding LB structure. We have performed
an X-ray scattering study of three LB films to
understand the nature of interfaces present in these
systems and to probe molecular arrangements in
these films. In the next section we have described
these films and in the third section we have outlined
the experimental details and the formalism used to
analyse the measured X-ray scattering data. In the
last section the main results are discussed.
3. X-ray scattering study
X-ray specular reflectivity measurements were
performed on these films by keeping the angle of
incidence (a) equal to the angle of reflection (b)
while the diffuse scattering data were taken by
keeping these angles unequal [3,5]. The data was
collected using a triple axis spectrometer (optix
X-rays obtained
microcontrole) with Cu K?
ꢂ
from a rotating anode generator (FR 591, Enraf
Nonius) and a Si(1 1 1) monochromator. The inci-
dent beam was collimated by slits having horizon-
tal and vertical apertures of 100 and 5000 lm,
respectively, with the horizontal aperture determin-
ing the width of the incident beam in the scattering
plane. In case of diffuse scattering measurements
the scattered beam was defined in the scattering
plane by a horizontal slit of aperture 100 lm,
placed in front of the detector. The vertical aperture
of the detector slit was kept wide open to effectively
integrate [3,5] the out-of-plane component of the
scattering.
2
. The LB films
Two LB films of cadmium arachidate (CdA),
each 9 monolayer (ML), were deposited on quartz
substrates from a spread monolayer of arachidic
acid (AA) on an aqueous solution of cadmium
chloride (4;10\ꢁM) at a surface pressure, temper-
ature and pH of 30 mN m\ꢂ (surface tension
4
2 mN m\ꢂ), 10°C and 6.4, respectively. The depos-
ition rate was 10 mm/min. Of these films one was
The specular reflectivity data indicate that the
intensity of the multilayer Bragg peaks in all
the films increase with increasing horizontal de-
tector slit width even beyond the beam divergence
width. Moreover in a log—log plot the scattered
intensity was found to decay linearly, with a slope
(g!1), as a function of the in-plane scattering
vector q , where g depends on q . These results
clearly indicate that we are dealing with scatter-
ing which has a strong diffuse component around
the specular ridge similar to that observed in scat-
tering from liquid surfaces [5,13] with logarithmic
exposed to H S gas for 60 mins. The details of the
ꢀ
experimental arrangement used to prepare these
LB films has been described earlier [11]. In the
UV—VIS absorbance data taken on these films the
absorption edge for the H S exposed film was
ꢀ
found to be at 455$5 nm indicating the formation
of nanocrystalline CdS in this film [10,11].
V
X
Ferric stearate (FeSt) was prepared by adding
a measured amount of ferric sulphate solution to
freshly prepared sodium stearate solution in hot,
distilled water until the residual solution was slight-