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HAL Id: jpa-00209938

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Submitted on 1 Jan 1985

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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�

(2)

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.

2014

Nous 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.

2014

Spin 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

(3)

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

(4)

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.

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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

(6)

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

5

with 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

(7)

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

s

with surface pressure for model 2.

Fig. 9.

-

Variation of the number of pairs of different type N12/Ns

s

with 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

-

0.10 dyne/cm. A’, half the experimental value. The

area of the vacancies is equal to A 1/6, the area per site.

For a symmetric model like our model 2, it is possible in some cases to have a first order critical

point c 1 determined by the conditions a

-

p y

aQ

=

~203C0

(~203C0)

=

0 and M

=

0 provided that such a point

~2 T

does not lie within the coexistence region of the second order transition. The conditions for the critical point correspond to QC1 1

=

1 /2 and

The parameters chosen for model 2 give for that point the coordinates T C = 103.3 K, 7rcl

=

1.12 dyne/cm, and 03C3C1

=

281.2 Ä2; it is located well

within the second order phase transition coexistence

region therefore it is not a stable state for this model.

Adjustable parameters necessary to locate this first order critical 10.5 dyne/cm, and point at TCt 1

=

300 K, nCt 1

=

O’Ct

=

140 A2 require such a high

interaction that the system is condensed even at

03C0

=

1 dyne/cm. Such an interpretation must be

dismissed

It is seen that the two models give predictions for

Ay Ayr Aye-

that d.

.

t: h

.

I

Au AT and A7r m that deviate from the experimental

AT’AT Aum

values in opposite directions; the two models are

in some sense extreme opposites and we might expect that intermediate models would give better

agreement with the experimental data.

We have examined other models not symmetric

with respect to the « magnetization » by allowing A2 to be different from A1 but the results deviate

even more from the observation. Other models exhi-

biting second order phase transitions with either

03B4A12 "# 0 or U,2 :0 0 or both # 0 have been exa- mined ; the slope of the critical line is not significantly

affected and we do not improve the fit significantly,

the main effect being the reduction of am ; one can

in fact fit am either at 0 °C at 28 °C but not at both

temperatures.

(8)

4. Conclusion.

The nature of the transitions given by the two models

considered is seen to depend upon the inclusion of vacancies as is made evident by (14) where A3

and K almost exclusively determine the critical and tricritical temperatures; reducing A 3 would make the critical pressure to grow indefinitely. On the con- trary, lattice models with no vacancies exhibiting

transitions usually predict pressures much lower than observed

,

The introduction of an area reduction due to nesting

when pairs form seems to provide an explanation

for the large anomalous compressibility with or

without a true pressure plateau after the transition when a second order phase transition takes place.

Model 2 in fact is compatible with the observed relaxations near the transition; moreover the area A3

that must be assumed is compatible with the size of triangles in the lattice used for the model.

Neither model is completely satisfactory as is

shown by the large deviations in the slopes of the

coexistence regions, from the observed value. Also both models predict a condensed area Qo around 80 A2 which is about one-half the value obtained

by extrapolating to n

=

5 the area measured by X-ray (2) for BH-n existing in the mesophase (discs irregularly spaced forming liquid-like columns) that

is n

=

7 and 8. Since the monolayers can be com- pressed to nearly 100 A2 before collapse, it is believed

that the chains in the monolayer are not extended

as they are in the mesophase but are instead in a

tighter configuration stabilized by the strong anchoring

of the C02 groups to the water substrate thus allowing

a smaller closed packing area.

The anomalous features observed on BH-5 are

also present for the other members of the BH-n

family and also for phospholipids, see references [8-10]

for the literature on that subject; phospholipids are

sometimes described [10] as a system where rigid

molecules undergo melting of their chains as the concentration is lowered and a model similar to ours could be used provided the differences in internal energy and entropy are included in the isotherm- isobar potential. Their transition could be partly explained by a nesting concommittent with the

ordering of the molecules through rigidization upon condensation thus showing an anomalous compres-

sibility after a transition where mostly vacancies are expelled and rigid molecules are pairing at a high

rate.

Of course, our models are not versatile enough

to explain the richness of features observed for the BH-n’s or for the phospholipids, hence we cannot

exclude a priori explanations based upon cooperative phenomena involving formation of clusters [11] leading

to continuous transitions that seem to have been

recently confirmed experimentally by electron micro- scopy diffraction studies upon phospholipid mono- layers transferred from water to solid substrates [12].

References

[1] RONDELEZ, F. and KOPPEL, D., J. Physique 43 (1982) 1371 ; see references to review articles therein.

[2] CHANDRASEKHAR, S., SADASHIVA, B. K., MADHUSU-

DANA, N. V., KUMAR, S., SASHIDAR, R. and VEN- KATESH, G., J. Physique Colloq. 40 (1979) C3-120.

[3] BELL, G. M., MINGINS, J. and TAYLOR, J. A. G., J.C.S.

Faraday I 74 (1978) 223.

[4] FIRPO, J. L., LEGRE, J. P., Bois, A. G. et BARET, J. F., J. Chim. Phys. 81 (1984) 113.

[5] RONDELEZ, F. and BARET, J. F., to be published in the

J. Physique.

[6] BOIS, A. G., PANAIOTOV, I. I. and BARET, J. F., Chem.

Phys. Lipids 34 (1984) 265.

[7] CAILLE, A., PINK, D. A., DE VERTEUIL, F. and ZUCKER- MANN, M. J., Can. J. Phys. 58 (1980) 581.

[8] PHILIPS, M. C. and CHAPMAN, D., Biochim. Biophys.

Acta 163 (1968) 301.

[9] NAGLE, J. F., J. Membr. Biol. 27 (1976) 233.

[10] ALBINET, G. and TREMBLAY, A.-M. S., Phys. Rev. A 27 (1983) 2207.

[11] GEORGALLAS, A. and PINK, D. A., Can. J. Phys. 60 (1982) 1678.

[12] FISHER, A. and SACKMANN, E., J. Physique 45 (1984) 517.

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