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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�
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.
2014La 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.
2014Formulae 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
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
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
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