II. THEORETICAL FORMULATION
Consider a fluctuating fluid membrane that is confined to two
interacting parallel walls 1 and 2. We denote by D their finite
separation. Naturally, the separation D must be compared to the bulk
membrane roughness, L01, when the system is
unconfined (free membrane). The membrane is confined only when the condition
L << L01 is fulfilled. For the opposite
condition, that is L >> L01, we expect
finite size corrections.
We assume that these walls are located at z =
-D/2 and z = D/2, respectively. Here, z
means the perpendicular distance. For simplicity, we suppose that the two
surfaces are physically equivalent. We design by V (z) the
interaction potential exerted by one wall on the fluid membrane, in the absence
of the other. Usually, V (z) is the sum of a repulsive and an
attractive potentials. A typical example is provided by the following potential
[22]
V (z) = Vh (z) +
VvdW (z) , (2.0)
where
Vh (z) =
Ahe-z/Ah (2.0) represents
the repulsive hydration potential due to the water molecules inserted between
hydrophilic lipid heads [22]. The amplitude Ah and the potential-range
ëh are of the order of : Ah ^, 0.2
J/m2 and ëh ^, 0.2-0.3 nm. In fact,
the amplitude Ah is Ah = Ph xëh, with
the hydration pressure Ph ^, 108-109 Pa. There,
VvdW (z) accounts for the van der Waals potential
between one wall and biomembrane, which are a distance z apart. Its
form is as follows
[ ]
H 1 1
VvdW (z) = - ,
z2 - 2
(z + ä)2 + (2.0)
12ð (z + 2ä)2
with the Hamaker constant H ^, 10-22 -
10-21 J, and ä ^, 4 nm denotes the membrane thickness.
For large distance z, this implies
Wä2
VvdW (z) ? z4 .
(2.0) Generally, in addition to the distance z, the interaction
potential V (z) depends on certain length-scales,
(î1, ...,în), which are the
interactions ranges. The fluid membrane then experiences the following total
potential
I D ) I D ) , -D
U (z) = V 2 - z + V
2 + z 2 < z < D 2 .
(2.0) In the Monge representation, a point on the membrane can be
described by the three-dimensional position vector r = (x,
y, z = h (x, y)), where h (x, y) E
[-D/2, D/2] is the height-field. The latter then fluctuates
around the mid-plane located at z = 0.
The Statistical Mechanics for the description of such a
(tensionless) fluid membrane is based on the standard Canham-Helfrich
Hamiltonian [9, 23]
? [ê ]
1-l [h] = dxdy 2
(?h)2 + W (h) , (2.0) with the
membrane bending rigidity constant ê. The latter is comparable
to the thermal energy kBT, where T is the absolute
temperature and kB is the Boltzmann's constant. There, W
(h) is the interaction potential per unit area, that is
U (h)
W (h) = L2 , (2.0) where
the potential U (h) is defined in Eq. (2), and L is
the lateral linear size of the biomembrane. Let us discuss the pair-potential
W (h).
K. El Hasnaoui et al. African Journal Of Mathematical Physics
Volume 8(2010)101-114
Firstly, Eq. (2) suggests that this total potential is an
even function of the perpendicular distance h, that is
W (-h) = W (h) .
(2.0)
In particular, we have W (-D/2) = W
(D/2).
Secondly, when they exist, the zeros h0's of the
potential function U (h) are such that
(D ) (D )
V 2 - h0 = -V 2 +
h0 . (2.0)
This equality indicates that, if h0 is a zero of the
potential function, then, -h0 is a zero too. The number of zeros is
then an even number. In addition, the zero h0's are different
from 0, in all cases. Indeed, the quantity V (D/2) does not
vanish, since it represents the potential created by one wall at the middle of
the film. We emphasize that, when the potential processes no zero, it is either
repulsive or attractive. When this same potential vanishes at some points,
then, it is either repulsive of attractive between two consecutive zeros.
Thirdly, we first note that, from relation (2), we deduce that
the first derivative of the potential function, with respect to distance
h, is an odd function, that is W'
(-h) = -W' (h). Applying this relation to
the midpoint h = 0 yields : W' (0) = 0. Therefore,
the potential W exhibits an extremum at h = 0, whatever the
form of the function V (h). We find that this extremum is a
maximum, if V ?(D/2) < 0, and a
minimum, if V ?(D/2) > 0. The
potential U presents an horizontal tangent at h = 0, if only
if V ?(D/2) = 0. On the other hand, the general
condition giving the extrema {hm} is
dV dh
|
????h= D 2 -hm
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dV =
dh
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????h= D 2 +hm
|
. (2.0)
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Since the first derivative W' (h)
is an odd function of distance h, it must have an odd number
of extremum points. The point h = hm is a maximum,
if
and a minimum, if
|
d2V dh2
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????h= D 2 -hm
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<
|
d2V dh2
|
????h= D 2 +hm
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,
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(2.0)
|
d2V dh2
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????h= D 2 -hm
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>
|
d2V dh2
|
????h= D 2 +hm
|
. (2.0)
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At point h = hm, we have an
horizontal tangent, if
d2V
dh2
????h= D 2 +hm
. (2.0)
d2V dh2
????h= D 2 -hm
104
The above deductions depends, of course, on the form of the
interaction potential V (h).
Fourthly, a simple dimensional analysis shows that the total
interaction potential can be rewritten on the following scaling form
W (h) kBT
|
D2Ö( = 1 h1n 1
(2.0) D, D,..., D J ,
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where (î1, ...,în)
are the ranges of various interactions experienced by the membrane, and
Ö(x1, ..., xn+1) is a (n + 1)-factor
scaling-function.
Finally, we note that the pair-potential W
(h) cannot be singular at h = 0. It is rather an
analytic function in the h variable. Therefore, at fixed ratios
îi/D, an expansion of the scaling-function Ö,
around the value h = 0, yields
W (h) kBT
h2
2 D4
= ã + (h4) .
(2.0)
K. El Hasnaoui et al. African Journal Of Mathematical Physics
Volume 8(2010)101-114
105
We restrict ourselves to the class of potentials that exhibit
a minimum at the mid-plane h = 0. This assumption implies that the
coefficient ã is positive definite, i.e. ã >
0. Of course, such a coefficient depends on the ratios of the
scale-lengths îi to the separation D.
In confinement regime where the distance h is small
enough, we can approximate the total interaction potential by its quadratic
part. In these conditions, the Canham-Helfrich Hamiltonian becomes
W0 [h] = 2 J dxdy
[1ê (?h)2 + uhl
, (2.0)
with the elastic constant
u = ã kBT
D4 .(2.0)
The prefactor ã will be computed below. The
above expression for the elastic constant u gives an idea on its
dependance on the film thickness D. In addition, we state that this
coefficient may be regarded as a Lagrange multiplier that fixes the
value of the membrane roughness.
Thanks to the above Hamiltonian, we calculate the
mean-expectation value of the physical quantities, like the height-correlation
function (propagator or Green function), defined by
G (x - x', y -
y') = (h (x, y) h
(x',y')) - (h (x,
y)) (h (x',y')) .
(2.0)
The latter solves the linear differential equation
(îc?2 + u)G(x -
x',y - y') = ä (x -
x')ä (y - y') , (2.0)
where ä (x) denotes the one-dimensional
Dirac function, and ? = ?2/?x2 +
?2/?y2 represents the two-dimensional
Laplacian operator. We have used the notations : = ê/kBT and u =
u/kBT, to mean the reduced membrane elastic constants.
From the propagator, we deduce the expression of the membrane
roughness
L2? = (h2)
- (h)2 = G(0,0) . (2.0)
Such a quantity measures the fluctuations of the
height-function (fluctuations amplitude) around the equilibrium plane located
at z = 0. We show in Appendix that the membrane roughness is exactly
given by
2
L2 = 12, (2.0)
provided that one is in the confinement-regime, i.e. D
<< L0?. Notice that the above equality
indicates that the roughness is independent on the geometrical properties of
the membrane (through ê). We emphasize that this relation can be
recovered using the argument that each point of the membrane has equal
probability to be found anywhere between the walls [24].
The elastic constant u may be calculated using the known
relation
L2 1 kBT = (2.0)
?8 ,urs .
This gives
u =
9 (kBT)2
êD4 . (2.0)
4
This formula clearly shows that this elastic constant decays
with separation D as D-4. The term
uh2/2 then describes a confinement potential that
ensures the localization of the membrane around the mid-plane. Integral over
the hole plane R2 of this term represents the loss
entropy due to the confinement of the membrane. The value (19) of the elastic
constant is compatible with the constraint (17).
Therefore, the elaborated model is based on the Hamiltonian
(13), with a quadratic confinement potential. We can say that the presence of
the walls simply leads to a confinement of the membrane in a region
K. El Hasnaoui et al. African Journal Of Mathematical Physics
Volume 8(2010)101-114
of the infinite space of perpendicular size L?.
We define now another length-scale that is the in-plane
correlation length, L?. The latter measures the correlations extent
along the parallel directions to the walls. More precisely, the propagator
G (x - x', y -
y') fails exponentially beyond L?, that is for
distances d such that d =
v(x - x')2
+ (y - y')2
> L?. From the standard relation
L2 ? = kBT
16ê L2 ? , (2.0)
we deduce
L
(2.0)
( ê )1/2
2
? = v3 D .
kBT
In contrary to L?, the length-scale L?
depends on the geometrical characteristics of the membrane (through
ê).
The next steps consist in the computation of the Casimir force at
and out equilibrium.
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