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Submitted on 1 Jan 1987

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Measures of integration in calculating the effective rigidity of fluid surfaces

W. Helfrich

To cite this version:

W. Helfrich. Measures of integration in calculating the effective rigidity of fluid surfaces. Journal de

Physique, 1987, 48 (2), pp.285-289. �10.1051/jphys:01987004802028500�. �jpa-00210441�

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Measures of integration in calculating the effective rigidity of fluid

surfaces

W. Helfrich

Institut für Theoretische Physik, Freie Universität Berlin, Arnimallee 14, D-1000 Berlin 33, F.R.G.

(Reçu le 3 juin 1986, accept,6 le 6 aotit 1986)

Résumé.

2014

La rigidité à la flexion de surfaces fluides est abaissée par des fluctuations hors du plan ; les auteurs qui

ont calculé cet effet trouvent des expressions qui diffèrent par un facteur numérique (1 ou 3). Nous comparons les

mesures de l’intégration (ou les représentations en modes) dans le cas d’une tige flexible, nous montrons pourquoi les

mesures de déplacement à une dimension ne sont pas adéquates, et nous examinons la mesure de la courbure pour les surfaces. Nous redérivons notre résultat antérieur (facteur numérique 1) par un couplage géométrique de modes de fluctuation de la courbure qui sont énergétiquement découplés.

Abstract.

2014

Formulae differing by a numerical factor (1 vs. 3) have recently been obtained by several authors for the decrease of the bending rigidity of fluid surfaces caused by out-of-plane fluctuations. We compare the measures of

integration (or the representations of the modes) for the example of the flexible rod, show why one-dimensional

displacement measures are inadequate, and examine the curvature measure for surfaces. Our previous result (factor 1) is rederived in terms of coupling by geometry of energetically decoupled curvature fluctuation modes.

Classification Physics Abstracts

68.10E

-

87.20C

1. Introduction.

In the last two years a number of authors [1, 5] have

calculated the softening of fluid membranes and inter- faces caused by out-of-plane fluctuations. The effective

bending rigidity K’ is predicted to obey

where K is the bare (or local) bending rigidity, kB Boltzmann’s constant and T temperature. The cutoff

wave vectors qm;n and q max are governed by the

dimensions of the surface and of the constituent

molecules, respectively. The numerical factor a has been found to be unity by the present author [1] and

three by the others [2-5].

All the theories start from the bending elastic energy per unit area

where cl and c2 are the principal curvatures, co the spontaneous curvature which we assume here to vanish, and K the elastic modulus of Gaussian curvature cl c2, The integral of g over the surface area represents the total energy of the system. We do not consider here the complicated case of nonvanishing surface ten-

sion [2, 3]. Central to all calculations is a coupling of

fluctuation modes with each other or with a stationary

deformation of the surface. It is treated to first order either by elementary means [1, 3] or in the language of

field theory and renormalization [2-5]. (In one example

both methods are applied and give the same result [3].)

The basic disagreement among authors lies, briefly, in

the « measure ». We mean the measure of integration

used to set up partition functions and the measure or representation used to define fluctuation modes and calculate the coupling between them.

The measure of most authors is displacement, either

normal to a flat base [2, 3] or normal to a curved base

representing the surface without short-wavelength fluc-

tuations [4, 5]. Like any measure referring to a fixed base, the two one-dimensional displacements omit

lateral motion. Such motion is inevitable as the real surface area over a given piece of base varies during out-of-plane fluctuations. In fact, the bending energy is generally calculated for the real area and on the

assumption that the surface is unstretchable, i.e. of fixed density. The neglect of lateral motion is particu- larly dangerous if displacement itself is the measure.

Our elementary calculation, in its first version [1a], employs director fluctuation modes. Actually, they are

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01987004802028500

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286

curvature modes as they satisfy the stated requirement

of being additive in the elastic strain which is curvature.

(At one point we wrongly invoke displacement to deal

with entropy. This is corrected in the Note added in

proof). The curvature modes are defined with respect

to a flat base area and are thought to couple through

the increase in real area over base area which they produce. In the second version [lb], concerning a spherical surface, we start with displacement modes.

The curvature measure is invoked to derive the changes

of mode entropy due to spherical curvature.

The purpose of the present note is twofold. Firstly,

the curvature measure is to be derived from the full

positional measure for the simple model system of an unstretchable rod, partly represented by a stiff polymer

chain. The rod, if restricted to a plane, is in some

respects equivalent to a membrane with curvatures in

one direction only. The model is of course not novel, but prepares for the use of the curvature measure in connection with surfaces. Also, it is used to indicate the failure of the one-dimensional displacement measures.

Secondly, we wish to deal with the curvature measure

in more detail and rigor than before. The curvature fluctuation modes of an originally flat surface are

described such that they are decoupled like those of the rod. The previous value of the effective rigidity (a =1 ) is obtained solely from the deformed geometry of the fluctuating surface. It is hoped that the exposition settles the controversy about the measure.

2. The rod in a plane.

An instructive, discrete model for the rod is the stiff

polymer. It permits us to write down precise partition

functions in terms of mass points. For the sake of simplicity, the monomers are taken to be single mass points, thus having no moments of inertia. We imagine

a sequence of N + 1 equal masses. Their position

vectors are

r, ( j

=

0,..., N ) , with r. being fixed. The

bond vectors are a, = r, - rj - 1 ( j =1, ..., N ) . We adopt a vector ao ending in ro to fix the direction of the

nearly straight chain. Bending vectors may be defined

as kj = (aj , Iaj _, 1 - ajlaj) a ( j = o, ..., N -1 )

where a is the time-averaged spacing of subsequent

mass points. The vector kj is the discrete equivalent of

the curvature vector of differential geometry if a is constant, as we will stipulate immediately. Cohesion

and stiffness of the chain may be enforced by a potential energy of the type

The complete partition function of classical statistical mechanics then takes the form

where f3 =1/kB T. The thermal de Broglie wavelength

A of the mass points is used to express the volume of the

unit cell in configurational space, À 3N. The factor will be dropped in the following. By adding the mass points

one after the other it is easy to see that the position

vectors can be replaced by the bond vectors as inte- gration variables so that Zr becomes

The fluctuations of the bond lengths are assumed to be

very small. We integrate them out and put aj = a

=

constant. This leads to modifications of Zr and Za : The potentials u ( aj) drop out and 8j is restricted to the surface of a sphere of radius a. An interesting third

form of the partition function,

can now be obtained by substituting a2 dkj - 1 for da,

and omitting constant factors. Naturally, k, is con-

strained through the fixed lengths of aj and a; + 1 so that

its end point describes a sphere.

The various constraints imposed by constant bond length (or line density) are difficult to handle in three-

dimensional space. The situation is simplified for the polymer in a plane. Its partition function may be

written as

where k, can be counted positive or negative depending

on whether the polymer turns left or right. Equation (7) is, of course, an approximation valid for stiff enough chains, i.e. (k?) ..,:a -2 (An exact form for more

flexible chains could be obtained by using bond angles.)

A continuum version of (7) is

This is just the partition function of the unstretchable rod in a plane. A finite set of integration variables

kj has now been replaced by a continuum of variables k

=

k ( s ), s being the arc length and L the total length

of the rod. The symbol 0 marks the measure of

integration, k. The two partition functions, discrete and

continuous, are practically equivalent if

E being the bending rigidity of the rod.

The advantages of the curvature measure in writing

the partition function for the rod in a plane are obvious.

The constraint of no stretching is incorporated auto- matically, leaving k(s) to be an arbitrary function,

while the original function r (s) describing the rod’s

shape is under the constraint I drlds I = 1. This is a

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formal argument against the use of displacement

measures. Moreover, curvature is identical to the elastic strain. If Hooke’s law is valid, the fluctuation modes of k(s) as obtained by the usual Fourier

expansion are.completely decoupled energetically. The

modes can therefore be treated separately. The only coupling that may remain between them is through the

deformed geometry of the fluctuating rod.

The simple example of the unstretchable rod in a

plane may serve to recognize the most conspicuous shortcomings of the one-dimensional displacement

mesures. We consider first displacement normal to a

base line [2, 3]. The rod is restricted to the xz plane and

taken to coincide with the x axis in the absence of fluctuations. The small distances II z of the fluctuating

rod from this base are expressed by u

=

u (x ) . Let us imagine a short-wavelength mode ul being superim- posed on a region of practically uniform slope du2/dx

associated with a long-wavelength mode U2’ If the

amplitude of the former is very small, material transport along the sloping line may indeed be ignored as it varies

with the square of the amplitude. However, one has to take into account that the material displacement as-

sociated with the new mode will be orthogonal to the sloping line. Therefore, the physical displacement is

smaller by the factor [1 + ( du2/dx ) 2] -1/2 than that

measured in u. Being proportional to the square of the

slope, the correction couples the modes in the lowest order possible, so it cannot be disregarded. One could hope to avoid the failure by choosing as measure the

displacement f normal to a curved base line [4, 5].

Vnfortunately, even a single fluctuation mode then ihV-61ves motions along the base which are proportional

to its amplitude. This is because the half-waves of, say,

f = f a sin ( qs ) on the convex side require more

material than those on the concave side of the curved base. The corrections of the displacement measure,

which also depend on sin (qs), produce a nonnegli- gible coupling of lowest order.

3. Curvature measure for surfaces.

It seems clear now that one should not use one-

dimensional displacement measures to deal with the

(possible) coupling of bending fluctuations either of rods or of fluid surfaces. How can one extend the curvature measure to unstretchable fluid surfaces ? The

only linear invariant to be formed from the two- dimensional tensor of surface curvature is its trace,

c = cl + C2 [6]. We adopt it as measure of integration.

One can in general neither choose c, and c2 separately

nor control the orientation of the principal axes. A

visual way of realizing this is to build the surface by placing mass points one after the other along an edge of

the surface. Evidently, the height of a new mass point

relative to some neighbours that are already there is the only available degree of freedom apart from fluidity

and determines the local curvature c. It is not possible

to propose for fluid surfaces a molecular model of similar precision as that for the polymer chain, though

lattice models may be helpful to some extent.

We want to transform a flat and square piece of

surface coinciding with the xy plane into a slightly

undulated surface in roughly the same location. Denot- ing the positions on the flat surface by x

=

6, y

=

q, we specify everywhere on it the curvature c ( § , q which

a surface element is to assume and look for a mapping r ( 6, q ) which also conserves local density and is

invertible. The three demands can, in principle, be simultaneously satisfied as the fundamental theorem of surfaces allows for exactly three degrees of freedom in surface mapping [6]. The conservation of local density

may require the material to shear in its plane, which is

without consequences in a fluid. A one-to-one mapping

can be achieved, e.g., by stipulating that the material transport asociated with the transformation is irro- tational in the xy plane. Other prescriptions for the

local rotations are equally acceptable. However, one-

to-one mapping itself is a prerequisite on physical grounds, since different parts of the fluid are indisting-

uishable which means that a particular shape of the

surface must not be counted more than once.

The three conditions imposed on r ( §, 11) may be summarized by the equations

where the subscripts designate derivatives. A Fourier

expansion of c ( 6, q ) defines surface fluctuation modes that are energetically decoupled like those of the rod in a plane. Accordingly, the modes can be treated separately and there is no need for the partition

function formalism. The decoupling may not be perfect

if the usual periodic boundary conditions are to be satisfied for r as well as for c, here with an adjustable

square frame to conserve total membrane area. We

expect the effects of the boundaries to be negligible for

stiff and large enough surfaces. (It is certainly possible

to map any undulated surface back onto the flat square, but this may involve the curvature mode of zero wave

vector.) The only important mode-mode coupling that

remains is by geometry, i.e. by the deformation of the surface. It will lead us to rescale lengths and to

renormalize directors.

To begin with, the ripples representing the fluctua- tions contract the adjustable square frame. The ratio of fixed real area A to variable base area A’ is, to first order, given by

1 -1

---

where the director n obeys

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288

and is defined such that nz > 0. Equation (11) has been

derived many times and in different ways [7]. For a

derivation in terms of curvature we may use the Fourier

expansion

where p

=

( § , 7y) . Also needed are the equipartition

theorem

the director amplitude

the first-order ansatz

and periodic boundary conditions. In the last two

equations we ignore the difference between a wave

vector on the flat base and its counterpart on the

deformed surface. Evaluating the sum in (16) by means

of the usual integral and considering the cutoff wave vectors result in (11).

The consequences of rippling for curvature elasticity

may be conveniently studied for a mode of minimum

wave vector A with A = 2 ’IT / A - 112. If no other modes

are excited equations (14) and (15) prescribe :

where the minute base contraction due to the A mode is

disregarded. This has to be compared with the situation where all the other modes are released. Marking quantities that refer to the rippled surface produced by

the other modes with a prime and using [8] the generally valid relationship c = nx, x + ny, y, we have

c =A.n =A’.n’ (18)

The wave vector and, in compensation, the director

amplitude are rescaled in the last form which is a first- order approximation. Accordingly, (17) may be re-

written as

a L 1

The director has to be averaged over the ripples (except

the A mode) and subsequently brought back to unity.

The renormalized director amplitude of the A mode is

Inserting tA’ and A’ from (11) in (19), one arrives at

, -

m

where

Comparison with (19) shows K’ to be the effective rigidity felt by the A mode. The result confirms

equation (1) and, in particular, a = 1. The mean-

square displacement uA’ in z direction associated with

tA’ is readily seen to obey

with the same effective rigidity.

If base area rather than real area is held constant and if wave vectors always refer to the base, as in a similar

calculation of the effective rigidity [la], there is a coupling between modes through the increase in real

area which appears to be energetic. Shrinking the

fluctuating membrane, i.e. rescaling it in all three space dimensions, until its real area reaches the size without fluctuations, leads back to coupling by geometry. (Note

that the bending elastic energy is scale invariant.) The previous derivation avoids the problems of periodic boundary conditions, but is based on poorly defined

modes. However, the differences between the two

methods, including small changes in the cutoff qmax’ do

not alter the effective rigidity in these first-order calculations.

The picture of coupling by geometry cannot be maintained in the presence of a stationary curvature.

We may think, e.g. of a closed sphere or a surface kept

between concentric cylinders of sufficient spacing to permit out-of-plane fluctuations. As the fluctuations reduce the effective rigidity they will be enhanced by

the externally imposed curvature. The decrement of the rigidity can now be deduced from the increase of mode entropies due to the enhancement. We have shown for the sphere [1b] (and checked for the

cylinder) that this method gives the same effective rigidity as coupling by geometry.

The notion of curvature modes interacting with an externally imposed curvature may be used to disprove

Kleinert’s [5] claim that out-of-plane fluctuations also affect the modulus of Gaussian curvature, K. According

to the energy density (1) there is no interaction between pure saddle curvature, c2

= -

cl, and a curva- ture fluctuation mode. If the presence of the saddle does not change the mean-square amplitudes of the

modes there can be no effect on K. For the total free energy of the fluctuating spherical surface Kleinert [5]

obtains the same result from calculating rc’ and K’ in

the displacement measure as we do from deriving

K’ alone in the curvature measure. The coincidence could be related to the fact that our calculation of the effective rigidity of the sphere [1b] is, formally, insensi-

tive to whether curvature or displacement is regarded

as measure.

4. Conclusion.

The present analysis confirms the idea that the natural

measure in dealing with fluctuations is the elastic strain.

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The representation by strain is expected to give de- coupled fluctuation modes whenever Hooke’s law is valid. Incidentally, it also implies that the mean-square

amplitudes of the modes are all equal, i.e. independent

of wave vector. It is surprising that even a system as complex as a fluid surface fluctuating in three-dimen- sional space appears to obey these rules.

The curvature measure for surfaces may eventually

need a better molecular foundation than that sketched above. Also, the residual mode-mode coupling caused by periodic boundary conditions may be worth closer examination. However, there can be little doubt that

displacement measures are unsuited for studying the possible coupling between out-of-plane fluctuation modes. Actually, they may simulate a coupling where

none exists.

The situation is different if a fluctuating fluid mem-

brane is under lateral stress or subjected to a restoring

force that tends to keep it in a plane. Curvature may still be a good measure, but now the fluctuation modes

are coupled even in this representation.

Acknowledgment.

I am grateful to Dr. D. Forster for numerous, mostly

controversial discussions.

Note added in proof: Papers known to me only as preprints at the time of writing reconsider the softening

of membranes [9] and introduce a concept similar to effective rigidity into the theory of strings [10]. Newer

papers deal with strings [11] and membranes [12, 13].

All authors find a

=

3 except one who obtains

a = 1 [13]. See also a recent review [14].

References

[1a] HELFRICH, W., J. Physique 46 (1985) 1263.

[1b] HELFRICH, W., J. Physique 47 (1986) 321.

[2] PELITI, L. and LEIBLER, S., Phys. Rev. Lett. 54

(1985) 1960.

[3] SORNETTE, D., doctoral thesis, Nice, France (1985).

[4] FÖRSTER, D., Phys. Lett. 114A (1986) 115.

[5] KLEINERT, H., Phys. Lett. 114A (1986) 263.

[6] See textbooks on differential geometry.

[7] HELFRICH, W., Z. Naturforsch. 30c (1975) 841 ; BROCHARD, F., DE GENNES, P. G. and PFEUTY, P.,

J. Physique 37 (1976) 1099 ;

HELFRICH, W. and SERVUSS, R. M., Nuovo Cimento D 3 (1984) 137.

[8] See, e.g., reference [1a].

[9] KLEINERT, H., Phys. Lett. A 116 (1986) 57.

[10] POLYAKOV, A. M., Nuclear Phys. B 268 (1986) 406.

[11] KLEINERT, H., Phys. Lett. B 174 (1986) 335.

[12] DAVID, F., Europhys. Lett. 2 (1986) 577.

[13] FORSTER, D., Europhys. Lett., submitted.

[14] PELITI, L., Physica 140A (1986) in press.

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