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Description of monolayers of discotic molecules at air-water interface with spin one models including
vacancies and nesting of pairs
M. Banville, A. Caille, G. Albinet
To cite this version:
M. Banville, A. Caille, G. Albinet. Description of monolayers of discotic molecules at air-water
interface with spin one models including vacancies and nesting of pairs. Journal de Physique, 1985,
46 (1), pp.101-107. �10.1051/jphys:01985004601010100�. �jpa-00209938�
Description of monolayers of discotic molecules at air-water interface with spin one models including vacancies and nesting of pairs (*)
M. Banville, A. Caille
Département de Physique, Université de Sherbrooke, Sherbrooke, Québec J1K 2R1, Canada and G. Albinet
Département de Physique des Liquides, Université de Provence, 13331 Marseille Cedex 3, France
(Reçu le 9 juillet 1984, accepté le 12 septembre 1984)
Résumé.
2014Nous proposons des modèles de gaz sur réseaux pour essayer de décrire les isothermes de compression
de monocouches constituées de molécules de benzène-hexa-n-pentanoate (BH-5) disposées sur support aqueux.
Ces modèles sont résolus par la méthode de Bragg-William et ils permettent de tenir compte des lacunes, d’une réduction d’aire du coeur dur moléculaire suite à un emboîtement de paires. Nous considérons plusieurs méca-
nismes de formation des paires donnant des transitions tantôt du premier, tantôt du second ordre.
Abstract.
2014Spin one models based upon a lattice Bragg-William’s method are applied to the description of the surface-pressure isotherms of disc-like molecules of benzene-hexa-n-pentanoate (BH-5) forming monolayers at
air-water interface. The models include vacancies and consider a reduction of hard core area due to nesting when pairing occurs. Various assumptions about the way pairs form lead to different models exhibiting either first order
or second order phase transitions.
Classification Physics Abstracts
87.20C
1. Introduction.
Disc-like molecules of benzene-hexa-alcanoates have been shown [1] to form stable Langmuir monolayers behaving in many respects as monolayers of fatty acids.
The benzene ring plays the role of the polar head group while the alcanoate chains that of the long aliphatic
tails. These results indicate that the benzene rings lie
flat at the interface. The projection of the molecular diameter onto the interface is practically identical to
the lattice spacing measured in the liquid-crystalline
columnar mesophases formed in bulk whenever they
exist [2]. The area-pressure isotherms exhibit the well known three states characteristic of liquid-condensed, liquid-expanded and gaseous films according to
surface concentrations and temperatures.
Comparison between the lengths of the alcanoate chains deduced at equilibrium spreading pressure 1te and from molecular models show that the chains
are not fully extended at least beyond the fifth or
sixth methylene group and that there is a certain
chain rigidity which prevents the first methylene
groups to stand directly upright For BH-5, there is
some indications that their fully extended length
is about 1.5 times their length at 03C0e.
A lattice model proposed by Bell et al. [3] with
two types of particles differing by their orientations
including vacancies gave a second order phase
transition but did not explain the very large com- pressibilities after the transition as we compress the system.
The purpose of the present work is to offer an explanation for the very large compressibility after
the main transition as we compress monolayers
of BH-5 molecules. We propose spin one models
similar to Bell’s [3] and we assume further that an area reduction occurs when pairs are formed in some
relative orientations [4]. We consider here two diffe- rent models which differ by the way pairing occurs
between molecules. In part 2 we will discuss the fea- tures common to the two models followed by a description of their differences. The first model,
called model 1, is based upon an assumption for pair
formation that is not symmetric with respect to the change of sign of the so-called «magnetization»
order parameter, (to be defined later) hence leads (*) This research was partially supported by the Natural
Sciences and Engineering Research Council of Canada, and
le Fonds FCAC of Quebec.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01985004601010100
102
to a first order transition. The second model assumes a symmetric mechanism as in Bell’s model allowing
for a second order phase transition. In part 3, the parameters for the two models are determined to
give the best agreement with the experimental data;
the results are analysed and compared in part 4.
The experimental area-pressure isotherms for
benzene-hexa-n-pentanoate (BH-5) used for this study
were measured [5] by the movable barrier method for several temperatures between 0 °C and 28 °C ; they
are shown on figure 1. Important relaxation times
were observed near the main transition especially
for the lowest temperatures. A real plateau is never
observed after the transition although it is nearly
so for the lowest temperatures.
Fig. 1.
-Surface pressure isotherms of benzene-hexa-n- pentanoate for temperature 1) 0.6, 2) 5.4, 3) 10.4, 4) 15.0, 5) 20.9, 6) 24.9, 7) 27.2, 8) 28.6, and 9) 31.5 °C.
The experimental procedure used to observe the relaxations in the transitions is the same as the one
described for fatty acids in reference [6].
2. The models.
We consider models in which rigid molecules are
assumed to be in one of two orientations with respect
to the triangular lattice depicted in figures 2. The
lattice is introduced for the ’purpose of facilitating
the counting of configurations and to take into
account some of the local order; it is important
to keep in mind that there exists no substrate lattice.
The lattice sites also approximately take into account
the hard core repulsive interaction between molecules.
Molecules in the first orientation, called a have chains
pointing towards the middle of the lines joining the
lattice points, those in the second, called P, have
chains pointing to the lattice points.
Vacancies or unoccupied triangles are called y.
An index i
=1, 2, 3 will be used to designate the
states a, 03B2 and y respectively. A given configuration
for the system will be specified by the numbers N1 1
and N2 of molecules in the two orientations and the number N3 of vacant sites.
Provided we assume that the extra entropy due
to the presence of molecules in the orientation P
does not stabilize a mixed configuration, the fully
condensed state will be formed when all the mole- cules are in the orientation a. At other concentra-
tions, vacancies, a-a, a-fl, and p-p pairs will be present The area for the vacancies will be A3, and A1 = A2
will be the area of isolated molecules in either orien-
tation ; differences in hard core area are assumed to appear when pairs are formed due to nesting of
the radially extending chains leading to an area
reduction 03B4Aij when a molecule of type i pairs with
a molecule of type j.
The total area for a given configuration of N
molecules is
where J is the average area per molecule and Nij
are the number of i-j pairs averaged over a statistical ensemble of configurations characterized by N19 N2, N3. We work with a statistical ensemble where the number of molecules is fixed but the area varies;
this is the isothermal-isobaric ensemble [7]. The probability Pi of occupation of a given site in the ith state is given by
not taking into account correlations. Here, z
=6 is the number of sites occupied by a molecule and
N.,
=zN + N3 is the total number of sites. Simi-
larly, the numbers of pairs are given by
where z
=6 is the coordination of a molecule in that case.
The models being analog to an Ising spin one system, it is desirable to introduce order parameters M and Q that are the analogs of the magnetization and
the proportion of occupied sites respectively as
The probabilities expressed in terms of M and Q
are
and the area per molecule is
The isotherm-isobar potential [7] describing the equilibrium of this system will be
where p is the chemical potential per molecule whose minimum with respect to M and Q at constant and T determines the equilibrium configuration, H;n, is the energy of interaction between pairs
and S is the entropy of the system
It is convenient to introduce factors Uij that will
be used to define different models involving a single adjustable parameter K such that
When the area reduction terms in [8] are included
with the interaction terms, the interaction is seen to be renormalized; we define a renormalized inter- action
where To is room temperature.
We rewrite (7) in terms of the probabilities Pi
The pressure isotherms may be obtained by eva- luating from (6) after the values of M and Q mini- mizing (12) for fixed x and T have been found
The first model, called model 1 is based upon the type of pairing depicted on figure 2-a, a-a pairs
share 4 alcanoate chains, Lx-P pairs share 3 chains and fl-fl pairs share only two hence the a-a Van der
Waals bonds are expected to be stronger than a-03B2
bonds and a-fl bonds stronger than P-P bonds. The
model is rather insensitive to the exact relative values of the interaction parameters Kij as will be explained
in the discussion, hence we select a priori the following
relative values U11 = 3, U12 = 2, U22
=1. We
assume no area reduction (03B4A22
=0) when P-P pairs form and the same area reduction 03B4A 11
=03B4A 12
for a-a and cx-P pairs; this is suggested by a crude geometrical model of nesting and this assumption
will be later justified in the discussion.
For this model, the potential (12) is not an even
function of the « magnetization » M since K 11 # lz 22
and we can immediately predict that it will lead to a
first order transition.
Model 2 is based upon the pairing depicted on figure 2-b; a-a pairs and P-P pairs share 4 alcanoate
chains and cx-p pairs share 3 chains; pairs of similar
molecules will have a higher Van der Waals inter- action and will exhibit the same area reduction hence
we set U11
=U22 and A11
=6A22- We further
assume no interaction ( U 12
=0) and no area reduc-
tion (ðA12
=0) for Lx-# pairs; this assumption is
seen in part 3 to be consistent with the adjustment
of the parameters that give the best fit to the experi-
mental data. This model gives a potential (12) which
is symmetric under the inversion of the sign of M
Fig. 2.
-Configurations of BH-5 molecules a and {1, and vacancies y showing various types of pairing on a triangular
lattice : a) for model 1, b) for model 2.
hence second order phase transitions are possible
with this model.
104
3. Effect of the adjustable parameters.
3.1 MODEL 1. - For model 1, the isotherm-isobar potential (12) is seen to ccniain four adjustable para- meters, namely A1, A3, Ö II t and KlkB To. We will
select KlkB To in such a v ay as to obtain the critical temperature around 28 °C. Now there are a number of features in the experimental surface-pressure iso-
therms that can be used to determine the three remain-
ing parameters A 1, A 3 and 6A 11. We depict on figure 3
Fig. 3.
-Characterization of the surface isotherms at critical temperature by the critical area (Jc and critical pressure 1tc, and the extremities Qp and am of the coexistence
region at some temperature T.
the parameters nc, ac and Tc that characterize the critical point, the limits ap and am of the coexistence
AT A7T
.region, the variations - # and An near a given
temperature lower than Tc; Aa
=am - ap, and An is the rise in pressure in the coexistence region
for a variation AT of the temperature. We also exa- mine Anm/Aam, the slope of the coexistence line.
The experimental data on figure 1 suggest the
following values for those parameters : nc
=10 ± 1 dynejcm, Ue
=150 ± 5 A2, Tc
=28 ± 5 °C,
ap =130±10A2, am =250±5A2 A a 4.5+
up = 130 :f: 10
,m
,2iT
A2 An A7rm
0.5 JOC, " N-T
=0.12 +
-0.02 dyne/cm. OC, Y /
’and Aorm OQ m
=-
0.05 ± 0.002 dyne/cm. A2.
The area cho per molecule in the fully condensed
state can be obtained by setting P,
=1, P2
=P3
=0 yielding
When the pressure isotherms are calculated
requiring the critical temperature to be Tc
=28 OC,
the critical pressure is numerically seen to depend
almost exclusively upon the area A 3 of the vacancies :
We take 1tc
=10 dyne/cm from the data, hencf A3
=9.7 A2 from (14).
We also notice that the critical area (J c depends
almost entirely upon the values of A1 and ao. When
we require the fit to be best near condensation, we
find the approximate relation
to hold, where Qo is defined through (13) and the value of Jo
=80 A2 is nearly independent of the values of
A1 and 6A 11 . We take the critical area ac
=150 A2
from the data, hence A1
=115 A2 from (15), and 8A 11
=11.6 A 2 from (13). There is another relation that is seen to hold between the adjustable para- meters from the constraint T,
=28 °C; it is
that determines uniquely the interaction parameter
kB K To = 1.116, using A3 =9.7A 2 and 03B4A 1 1 = 1 1 .6 A2.
A slight readjustment of those parameters pro- vides a better fit with the width of the coexistence
region ; we show on figure 4 the pressure isotherms
Fig. 4.
-The model 1 area-pressure isotherms for T =0 °C to 28 °C by steps of 4 °C for the following values of the adjustable parameters : A 1
=125 A’, A 3 = 9.7 A2 ,
for T
=0 °C to 28 °C by steps of 4 °C calculated with the parameters A1
=125 A2, A3
=9.7 A2, ball
=15A2, kB K To
=1.092. The limits of the coexistence
B 0
region are i
0.132 dyne/cm.
in good quantitative agreement with the experimental
d Au .
in d I.. a reement but the
data, ET- IS in good qualitative agreement but the
A7r.
d 2 ,
slope e Q - - !.lam 0.0208 dyne/cm. A is too small by a
factor 2 and the area of the vacancies compared to A1/z, the area per site, is too small by a factor 2.
The examination of the way the populations of
molecules and pairs vary as we compress the system clarifies the nature of the transition. We have shown
on figures 5 and 6, the variations of N 11 and N 12
Fig. 5.
-Variation of the number of pairs of the same type N11/Ng
5with surface pressure for model 1.
Fig 6.
-Variation of the number of pairs of different type N,21N. with surface pressure for model 1.
with pressure. At the critical point, Z 2 1 N2 - = 2.25 and N. 2013
=5.62; the degree of ordering is important as
well as the proportion of vacancies. At a temperature
N N3
near 0 oC, at N ’ = 1.50, and N3 19.1 ; at up’
N1 NN2 N
-
=3.07, and L3 - 4 hence the main transition
2013
=3.07, and 2013
=1 54 ; hence the main transition
N2 N
is dominated by the expulsion of vacancies. The
number of pairs at am are N 11 =0.011 and N 12 _
NS NS
0.014; at 03C3p N-11 0. 135 and N12
0.087; hence 0.014;
’at up’ NNs s 0.135 and N12 - . N s 0.087;
,he n ce
the expulsion of vacancies is accompanied by ordering (i.e. : formation of a-a pairs); the number of a-fl pairs stays relatively small as can be seen on figure 6
and this explains why the model is not sensitive to the exact values of K12 and K22 as long as they are
smaller than K 11; the same remark holds for the difference between bAl2 and 03B4A11 ; the model is not sensitive to a variation of 6A 12
.Similarly, the nature of the changes in the com- pressibility anomaly region between up and the area
where the monolayer collapses may be clarified;
N1/N2 changes from 3.07 to 4.8 from up to collapse,
and N3/N changes from 1.54 to 0.60, hence the expul-
sion of vacancies is $till the dominant mechanism
compared to the ordering. Near T
=0 °C, the number
of pairs N11/Ng increases from 0.135 to 0.26 and
N12/Ns increases from 0.087 to 0.12 as we go from up to the collapse of the monolayer; the ordering is accompanied by the area reduction. If we extra-
polate the model to pressures above collapse, 1V12/1Vs
starts decreasing towards zero past 20 dynes/cm
while N11I1Vs keeps increasing towards its limiting
value of 0.5 indicating that the fully condensed state
if is existed would be completely ordered and not
a mixed phase.
3.2 MODEL 2.
-Model 2 gives isotherms with a very small slope after the transition as we compress
provided we are close or below the tricritical point indicating that the tricritical temperature is pro-
bably somewhere between 00 and 28 °C. There is a
possibility to go directly from an isotropic phase
to an ordered phase with a plateau having finite slope or from the isotropic phase to the ordered phase through a coexistence region with a true plateau.
In model 2 we also have four adjustable para- meters namely A 1, A 3, bA l l, and K/kB To and we
use the same criteria as for model 1 to find the values
giving the best fit to the experimental data. It is
seen that the slope of the critical line is quite insensi-
tive to the value of the parameters therefore there remains some freedom to choose bAll and K/kB To.
We have shown on figure 7 the pressure isotherms for the following values of the parameters : A 1
=150 A2, A3 = 25 A2, 03B4A11 = 25 A2 and K/kB To
=2.0 (here U11
=U22 = 1, U12
=0, and bAl2
=0).
Equation (13) gives a condensed area ao
=75 A2
in that case. The nature of the transition is clarified
by the figures 8 and 9 where we have shown the variation of N11 and N12 with pressure respectively;
in the expanded phase, pairs of all types are in equal
number for a given pressure and ordering suddenly
takes place as a-a pairs rapidly form while a-fl pairs
106
Fig. 7.
-Model 2 area-pressure isotherms for T
=0 OC to 28°C by steps of 4 OC for the following values of the adjustable parameters : A1 1
=150 A2, A3 = 25 A2, bAi l
=25 A2, and K/kB To
=2.0.
Fig. 8.
-Variation of the number of pairs of the same type N11/Ns
swith surface pressure for model 2.
Fig. 9.
-Variation of the number of pairs of different type N12/Ns
swith surface pressure for model 2.
decrease in number leading to almost complete ordering near collapse of the monolayer.
The isotherms are closer together near transition
than observed, we obtain An/AT
=0.075 in quali-
tative agreement with experiment; e Qm/e T
= -0.76,
very much smaller than observed, and An m
2i (T-M
-