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Biophys J, April 1999, p. 2056-2071, Vol. 76, No. 4
i
,*
a
Svetina,*§ and
tjan
ek
*§
*Institute of Biophysics, A sufficiently large force acting on a single point of
the fluid membrane of a flaccid phospholipid vesicle is known to cause the formation of a narrow bilayer tube (tether). We analyze this phenomenon by means of general mathematical methods allowing us to
determine the shapes of strongly deformed vesicles including their
stability. Starting from a free vesicle with an axisymmetric, prolate
equilibrium shape, we consider an axial load that pulls (or pushes) the
poles of the vesicle apart. Arranging the resulting shapes of strained
vesicles in dependence of the axial deformation and of the area
difference of monolayers, phase diagrams of stable shapes are presented
comprising prolate shapes with or without equatorial mirror symmetry.
For realistic values of membrane parameters, we study the
force-extension relation of strained vesicles, and we demonstrate in
detail how the initially elongated shape of an axially stretched
vesicle transforms into a shape involving a membrane tether. This
tethering transition may be continuous or discontinuous. If the free
vesicle is mirror symmetric, the mirror symmetry is broken as the
tether forms. The stability analysis of tethered shapes reveals that,
for the considered vesicles, the stable shape is always asymmetric
(polar), i.e., it involves only a single tether on one side of the main
vesicle body. Although a bilayer tube formed from a closed vesicle is
not an ideal cylinder, we show that, for most practical purposes, it is
safe to assume a cylindrical geometry of tethers. This analysis is
supplemented by the documentation of a prototype experiment supporting
our theoretical predictions. It shows that the currently accepted model
for the description of lipid-bilayer elasticity (generalized bilayer
couple model) properly accounts for the tethering phenomenon.
A point-force acting on the fluid membrane of a
flaccid phospholipid vesicle is known to pull out a narrow bilayer tube
(tether) from the vesicle membrane (Waugh, 1982 In these experiments, the measurements are usually carried out when
tubular membrane extensions of sufficient length have already formed.
Variation of the tether width or the tether length provides the desired
mechanical deformation. For the interpretation of measurements, it is
generally assumed that the (often invisible) tether has a cylindrical
shape, and simple parametrical models are used to extract the values of
different membrane material constants from the measured data. The
experience from a large number of experiments, and the often good
agreement of the measured data with predictions of the parametrical
models indicate that the used procedures are sufficiently accurate to
fulfill the purpose that they were designed for. Yet the fundamental
questions why and how tethers form in the first place are not addressed
by these models. The interesting task to reveal the basic mechanisms of tether formation is left to studies using more general mathematical methods and, most likely, involving nontrivial numerical computations.
Such studies can be based on the existing broad knowledge about the
shapes of free flaccid vesicles. The shape variety of unsupported lipid
vesicles has been the subject of elaborate theoretical and experimental
research work (reviewed e.g., in Lipowsky, 1991 Only very recently, some of these tools were applied also to the shapes
of axially strained vesicles. Considering the stability of the
cylindrical section of a pipette-aspirated, tethered vesicle, it was
shown that the existence of tethers is consistent with the generalized
bilayer couple model (Bukman et al., 1996 The paper is organized as follows. The next section gives an overview
of the generalized bilayer couple model, i.e., of the elastic energy
contributions that determine the shape of a simple bilayer membrane,
and of the relevant constraints. The model specifications for axially
strained vesicles and the mathematical methods used to tackle the
resulting variational problem are explained in the following two
sections. Eventually, numerical results are presented and discussed.
The conclusions emphasize the implications of our results for related experiments.
In general, the shapes of flaccid vesicles are governed by the
elastic energy of the vesicle membrane. It is the sum of the local and
the nonlocal bending energy (Helfrich, 1973
eva 2,
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ABSTRACT
TOP
ABSTRACT
INTRODUCTION
GENERALIZED BILAYER COUPLE...
VESICLE DEFORMATION BY AXIAL...
VARIATIONAL PROCEDURES
RESULTS AND DISCUSSION
CONCLUSIONS
APPENDIX
REFERENCES
![]()
INTRODUCTION
TOP
ABSTRACT
INTRODUCTION
GENERALIZED BILAYER COUPLE...
VESICLE DEFORMATION BY AXIAL...
VARIATIONAL PROCEDURES
RESULTS AND DISCUSSION
CONCLUSIONS
APPENDIX
REFERENCES
). A variety of
experimental techniques using tether formation have been developed and
have substantially increased our knowledge about the mechanical
properties of lipid membranes. For example, tether-pulling experiments
provided accurate values for the local bending modulus of fluid
bilayers (Bo and Waugh, 1989
; Song and Waugh, 1993
; Heinrich and Waugh, 1996
), and they also allowed for the first measurements of the nonlocal
bending modulus (Waugh et al., 1992
; Raphael and Waugh, 1996
).
Furthermore, the interlayer drag coefficient characterizing the
frictional interaction between the two membrane leaflets when sliding
past each other was measured by tether formation (Evans and Yeung,
1994
). Recent long-term observations of slowly growing membrane tethers
could be interpreted by postulating an elastically driven, accelerated
flip-flop of lipids from the inner to the outer monolayer (Raphael and
Waugh, 1996
; Svetina et al., 1998
). Other sets of recent
experiments involved tethers that were caused by internal
structures like microtubules growing inside vesicles (Hotani and
Miyamoto, 1990
; Kuchnir Fygenson et al., 1997a
, 1997b
; Umeda et al.,
1998
). Beside these studies of artificial lipid membranes, a number of
tether experiments have been performed using biological cells,
revealing new insight in cell membrane elasticity (e.g., Hochmuth et
al., 1973
, 1982
, 1996
; Dai and Sheetz, 1995
). Recently, tethers pulled
from red blood cells provided a measurement of the interaction strength
between the plasma membrane and the underlying protein network (Waugh
and Bauserman, 1995
; Hwang and Waugh, 1997
).
; Sackmann, 1995
;
Svetina and
ek
, 1996
; Seifert, 1997
). A continuum mechanical model accounting for the double-layer structure of the
membranes of artificial phospholipid vesicles ("generalized bilayer
couple model", Evans, 1974
; Svetina et al., 1992
; Seifert et al.,
1992
; Bo
i
et al., 1992
; Wiese et al., 1992
; Heinrich et
al., 1993
) has been able to reproduce many experimental observations quite reasonably (e.g., Käs et al., 1993
; Miao et al., 1994
; Wintz et al., 1996
; Döbereiner et al., 1997
), and a general
picture of the shape behavior of free vesicles is emerging. Naturally, the theoretical work was accompanied by the development of mathematical methods for the appropriate description of closed surfaces
exhibiting the elastic properties of simple bilayer membranes.
). Starting more generally
from the well-known equilibrium shapes of axisymmetric free vesicles,
it is instructive to consider axial loads that pull or push the vesicle
poles apart. Modeling this situation, a preceding study
(Bo
i
et al., 1997
) was devoted to the physics of membrane
deformations caused by a force acting in one point, and to the
specification of an Euler-Lagrange variational procedure for this
case. However, concentrating primarily on the basic mechanisms of the
onset of tether formation, the calculations in that study were
restricted to prolate axisymmetric vesicle shapes containing a mirror
plane at the equator. Moreover, the stability of stationary shapes was
not analyzed, and numerical problems had limited the range of
considered deformations to moderate vesicle extensions. In the present
paper, we extend the analysis by allowing also for shapes with broken
equatorial mirror symmetry, and we show that these shapes actually
dominate the shape behavior of axially strained vesicles. Furthermore,
the Euler-Lagrange variational procedure used previously is now
supplemented by a Ritz method that we recently developed to describe
strongly deformed vesicle shapes. The combination of these two methods
has enabled us to study considerably larger deformations than before,
and to include a stability analysis of stationary shapes. With these
improvements, we may now systematically explore the shapes and shape
transformations of axisymmetric, axially strained vesicles. Although
the theoretical background as well as the basic mechanisms presented
earlier remain fully applicable, we are now able to specify the
predictions for related experiments more precisely. Performing the
numerical calculations for a realistic range of material parameters of
phospholipid membranes, the present results should be directly
applicable to experimental situations. Finally, we suggest a new
experiment and document a prototype version of it that has partially
inspired the present theoretical study.
![]()
GENERALIZED BILAYER COUPLE MODEL
TOP
ABSTRACT
INTRODUCTION
GENERALIZED BILAYER COUPLE...
VESICLE DEFORMATION BY AXIAL...
VARIATIONAL PROCEDURES
RESULTS AND DISCUSSION
CONCLUSIONS
APPENDIX
REFERENCES
; Evans, 1974
, 1980
;
Bo
i
et al., 1992
; Miao et al., 1994
) and reads, for
symmetrical bilayers,
(1)
The local bending energy Wb is the integral
of the squared sum of the two principal curvatures
C1 and C2 over the closed surface area A, multiplied by the local bending modulus
kc. The nonlocal bending energy
Wr is the energy of relative stretching of the
two layers with respect to each other. The difference between the areas
of the two layers is given by
where h is the distance between the neutral surfaces of
the layers. The equilibrium value of the area difference
(2)
A0 is defined for isolated monolayers. It
depends on the numbers of lipid molecules constituting the layers and
on the (relaxed) area per molecule. The nonlocal bending modulus is
denoted by kr.
The value of the nonlocal bending modulus kr can
be easily estimated to be a few times the value of the local bending
modulus kc (Waugh et al., 1992
). Therefore,
vesicle deformations are generally accompanied by comparable changes in
both the local as well as the nonlocal bending energy. Yet, although
name and definition of the nonlocal bending energy first appeared quite
some time ago (Evans, 1974
, 1980
; Helfrich, 1974
), its importance in
the mechanics of layered membranes has long been overlooked. The
different models of vesicle shapes that have been suggested and studied during the past two decades were mainly distinguished by the value used
for kr, with values ranging from zero to
infinity (e.g., Deuling and Helfrich, 1976
; Svetina and
ek
, 1989
; Seifert et al., 1991
; Heinrich et al., 1992
).
We emphasize that it was tether formation that answered the question
which of the existing vesicle-shape models is most adequate to describe
experimental observations (Bo
i
et al., 1992
). The first
measurements of the nonlocal bending modulus kr
by means of tether formation (Waugh et al., 1992
) provided also a
quantitative verification of the generalized bilayer couple model,
which is based on the energy expression given in Eq. 1. (For an early
account of the history of this model, see the Introduction of Heinrich
et al., 1993
.) Recently, it was demonstrated that the study of vesicle
shape fluctuations could also serve to test this model quantitatively (Döbereiner et al., 1995
, 1997
). The latter works adhere to the notion of the area-difference elasticity model (synonym to generalized bilayer couple model) that was developed independently (Seifert et al.,
1992
; Miao et al., 1994
) to improve the understanding of the budding
shape transition of free vesicles. It should be noted that, in that
model, the material parameter characterizing the nonlocal bending
energy is defined as kr/
.
To determine the equilibrium shape of a free vesicle, one has to minimize the elastic energy given in Eq. 1. Because the membrane tensions of free vesicles as well as of the strained vesicles considered here are always small compared to tensions that would cause a significant change of the membrane area A, we may take the area to be constant. Not allowing for changes in the osmolarity of the solution surrounding the vesicle, the vesicle volume V is also fixed. Therefore, the energy minimization has to be performed at constant values of these constraints. Stationary shapes are characterized by a vanishing first variation of the energy functional that includes the constraints via Lagrange multipliers. To decide whether a stationary shape corresponds to a minimum of the elastic energy, an appropriate stability analysis has to be performed.
The resulting equilibrium shapes of free vesicles have been arranged in
a V
A0 phase diagram of stable
shapes, which is in reasonable agreement with experimental observations
(Heinrich et al., 1993
; Miao et al., 1994
; Jari
et al., 1995
).
The two main regions of this phase diagram contain prolate and oblate axisymmetric shapes, respectively. Either region is further divided into subregions of shapes with or without equatorial mirror symmetry. Except for vesicles with very low volume-to-area ratios (Wintz et al.,
1996
), it has been shown that, for realistic values of the ratio
kr/kc, nonaxisymmetric
shapes are generally of little or no relevance as stable equilibrium
shapes (Heinrich et al., 1993
; Jari
et al., 1995
).
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VESICLE DEFORMATION BY AXIAL STRAIN |
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Based on the knowledge about unsupported vesicles, we study the following physical situation. Starting from a free vesicle with a known equilibrium shape, we consider two points of the vesicle surface that are moved apart by a force acting on these two points. The force may be a pulling force acting on the outside of the vesicle, or a pushing force exerted by an internal structure. Because the lipid bilayer is fluid, the vesicle initially will merely change its orientation until the two points span the largest possible distance between any two points of the vesicle surface. This reorientation does not cost energy, i.e., it takes place at infinitesimal force. Any further increase of the distance between the two points changes the vesicle shape and requires a finite force. If the free vesicle has a prolate axisymmetric equilibrium shape, the force will thus eventually act along the symmetry axis and pull the poles of the vesicle apart. We do not expect this deformation to affect the rotational symmetry of the vesicle. In the case of an oblate shape, however, the force will act on two points of the largest cross section perpendicular to the symmetry axis, and so, it will cause a nonaxisymmetric deformation. Yet even in this case, it seems likely that sufficiently high forces will eventually cause the deformed vesicle to become axisymmetric. However, the theoretical treatment of this case is considerably more difficult and is beyond the scope of this study. Considering only prolate shapes, the present analysis stays within the case of rotational symmetry of free as well as of axially strained vesicles.
Principally, there are two different ways to impose the axial vesicle
deformation considered here. They can be studied experimentally using
the techniques presented as prototype versions in Figs. 1 and 2. It
is important to note that these two cases correspond to different
thermodynamic potentials (cf. Fig. 3). In
the first scenario, the vesicle poles are clamped at two points
separated by a fixed distance (Figs. 1 and 3 A).
Experimentally, this can be achieved by using the (often unwanted)
property of lipid membranes to adhere to glass surfaces. Attaching a
vesicle membrane to the tips of two glass micropipettes (Fig. 1) allows
us to set the desired pole-to-pole distance Z and to monitor
the equilibrium shapes that the vesicle assumes at different given
values of Z. In this first scenario, the constant
pole-to-pole distance enters the theoretical description as an
additional constraint. It is incorporated in the calculations via an
adjustable Lagrange multiplier representing the force that maintains
this distance. The total energy is then identical with the membrane's
elastic energy. Alternatively, we may consider a constant force acting
on the poles, and a variable pole-to-pole distance that depends on the
value of this force (Figs. 2 and 3 B). In the experimental
example shown in Fig. 2, the applied magnetic field sets the force that
the paramagnetic bead exerts at the free vesicle pole. Increasing the
force results in longer axial vesicle extensions, which eventually
leads to the formation of a narrow membrane tether (invisible in Fig.
2) connecting the lemon-shaped main vesicle body with the pipette tip.
(Details of the experimental setup including a possible accurate measurement of the applied forces in the range of piconewtons can be
found in Heinrich and Waugh, 1996
.) In the thermodynamic description of
this case, the work done by the force contributes to the system's
total energy, and it has to be included in the energy minimization
(Podgornik et al., 1995
; Bo
i
et al., 1997
). The potential
energy due to the axial force is simply
|
(3) |
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VARIATIONAL PROCEDURES |
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The variational problem of minimizing the total energy in the
presence of constraints is tackled with two different mathematical methods. The first is the usual Euler-Lagrange formalism that requires
us to solve a higher-order Euler differential equation. Second, we
present a new Ritz method (cf. e.g., Courant and Hilbert, 1924
) that
expands the vesicle shape in a series of basis functions and searches
for those values of expansion coefficients that minimize the energy and
fulfill the constraints. The general theoretical background and
technical details of the application of the Euler-Lagrange procedure
to the problem of axially strained vesicles have been explained in
Bo
i
et al. (1997)
and shall not be repeated here. As an
exception, we recall an interesting analytical result of the
Euler-Lagrange formalism. Proper treatment of the boundary conditions
revealed that a finite force acting on a single point of the vesicle
membrane leaves the vesicle contour, as well as its first derivative,
continuous (smooth) at this point. The principal curvatures, however,
show a logarithmic divergence (Podgornik et al., 1995
). Technically,
this discontinuity is taken care of by an expansion of the Euler
differential equation at the poles. The resulting two-point boundary
value problem is solved numerically by a shooting-to-a-fitting-point
algorithm. Unfortunately, for larger deformations, this method becomes
extremely sensitive to the initial guesses of adjustable parameters,
and it usually fails already at quite moderate values of the
pole-to-pole distance. An additional deficiency is the lack of a simple
stability analysis of stationary shapes within this Euler method. The
Ritz method has enabled us to overcome most of these difficulties. Its
main drawback is that it is an approximate method. However, its
accuracy can always be tuned by the number of terms included in the
shape expansion, and by a suitable parametrization of the shape.
Furthermore, the accuracy of the Ritz method can be easily tested by
comparing the results of this method with those of the Euler-Lagrange
formalism in the range of vesicle extensions where both methods work.
The application of direct variational methods such as the Ritz method
to vesicle shape calculations is not new (see e.g., Heinrich et al.,
1992
, 1993
). A previously used Ritz method expanded the radial distance
between the vesicle surface and the origin of the coordinate system
(suitably chosen inside the vesicle) in a series of spherical
harmonics. Accordingly, the independent variables of the shape
parametrization were the spherical angles. That method has proven to be
a powerful tool to determine the equilibrium shapes of free vesicles of
arbitrary symmetry including their stability (Heinrich et al., 1993
),
and it also has provided new insight in the effects of thermal shape
fluctuations on the vesicle shape (Heinrich et al., 1997
). However, it
has performed poorly when applied to the elongated shapes studied here
because, at increasing pole-to-pole distance, these shapes more and
more tend toward (and eventually turn into) shapes that are not anymore single-valued functions of the spherical angles. We have therefore developed a new approach (considering for now only axisymmetric shapes)
that is based on a parametrization more suitable for strongly deformed
vesicles. Because the contour of a vesicle is always a single-valued
function of the arc length measured along the contour line, this arc
length is the most practical choice for the independent variable. It
turned out to be convenient to take the direction of the contour normal
(i.e., the angle between the normal and a reference direction) as the
dependent variable. This choice has provided a surprisingly robust way
to determine the axially stretched shapes of interest. Technical
details of this Ritz method are rather subtle and will be published elsewhere.
The results presented in the following were obtained by a combination of the Euler-Lagrange approach and the Ritz method. Less deformed vesicle shapes were mainly calculated by the more accurate numerical integration of the Euler differential equation. At the same time, these shapes were used to check the reliability of the Ritz method. We found that including the first 100 terms of the shape expansion in the Ritz method yielded results that were, in all checked cases, indistinguishable from the results of the Euler method. If not stated otherwise, we continued to use this number of terms when calculating the more strongly deformed shapes that are inaccessible by the Euler approach.
The constraints of constant membrane area and vesicle volume generally
complicate the stability analysis of stationary shapes within the Euler
method. For all shapes calculated within the Ritz method, we have
determined the local stability with respect to those (axisymmetric)
deformations that conserve the constraints using an improved version
(see Heinrich et al., 1997
) of the formalism developed originally in
Heinrich et al. (1992)
.
| |
RESULTS AND DISCUSSION |
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Dimensionless quantities
Inspection of Eq. 1 shows that the elastic energy is
scale-invariant, i.e., the equilibrium shapes do not depend on the
actual size of the vesicle. We may use this property to present our
results in a general, dimensionless fashion (cf. e.g., Heinrich et al., 1993
). As usual, we take the characteristic vesicle size to be the
radius RS of the sphere having the same surface
area as the vesicle. We introduce dimensionless quantities by a
normalization with respect to this sphere. To distinguish normalized
quantities from the respective original ones, we denote the normalized
quantities by small letters. Thus, for example, v
V/(
RS3) (relative vesicle
volume), a = 1
A/(4
RS2)
(relative surface area),
a
A/(8
hRS) (relative area difference of
monolayers), z
Z/RS (dimensionless
pole-to-pole distance), and so on. The normalized elastic energy
wel is measured in units of the bending energy
of a sphere (8
kc). With this, the relative nonlocal bending energy becomes wr = q(
a
a0)2, where
q is the ratio between the nonlocal and the local bending modulus, q
kr/kc. The dimensionless axial
force is defined as f
FRS/(8
kc) (cf.
Bo
i
et al., 1997
).
Phase diagram of stationary shapes (q
)
For the presentation of numerical results, it is useful first to
give a transparent overview of the relevant stationary shapes. This can
be achieved by arranging the stationary shapes according to their
geometrical characteristics into phase diagrams, ensuring that similar
shapes occupy adjacent locations in these diagrams. The membrane area
a = 1 is the same for all shapes due to the normalization. Thus, the stationary shapes of free vesicles may be
characterized by the relative volume v and the relative area difference
a. It is important to realize, however, that,
unlike the constrained vesicle volume,
a may change when
a vesicle deforms, as it represents the average curvature of the
vesicle shape (cf. Eq. 2). Its value can be determined by solving the
variational problem at given values of v and
a0. Naturally, the resulting equilibrium
value of
a depends on the ratio q between the
nonlocal and the local bending modulus. Choosing different values for
q, however, has the mere effect of remapping a given
stationary shape (with known
a) to a new value of
a0, whereas the overall catalog of stationary
shapes is not affected by the value of q. In other words, if
we consider two distinct vesicle populations with membranes characterized by different values of q, we will find that
any stationary shape obtained for one population will also be a
stationary shape for the other population. However, the
a0 values of two vesicles having the same
stationary shape will generally be different if the two vesicles belong
to different populations. This applies both to unsupported vesicles
(Heinrich et al., 1993
) as well as to axially strained vesicles
(Bo
i
et al., 1997
).
The fact that the catalog of stationary shapes does not depend on
q allows us to classify the stationary shapes in a general manner. For this, we first choose q to be infinitely large.
In practice, this means that the nonlocal bending energy is replaced by
a constraint enforcing
a =
a0. Then,
the two constrained geometrical parameters v and
a map the resulting stationary shapes of free vesicles
into a two-dimensional phase diagram. Unfortunately, the phase diagram
of stationary shapes of axially strained vesicles is three-dimensional,
with the pole-to-pole distance z as the third parameter. For
relative volumes not too small, however, we expect the general shape
behavior to be similar at different volumes. To study this behavior
qualitatively, we may thus inspect a constant-volume cut through the
three-dimensional phase diagram.
The z
a phase diagram resulting from such a cut
at v = 0.95 is shown in Fig.
4, A and B. It
includes information about the stability of stationary shapes at
q
. Testing the stability for q
is
useful because switching to more realistic, finite values of
q merely adds the degree of freedom to adjust
a for the same stationary shapes (cf. Heinrich et al.,
1993
). Thus, shapes that are unstable at q
cannot be
stable at finite q, and so they need not concern us any
further. In contrast, the stable stationary shapes of Fig. 4 may become
unstable with respect to
a changes, and so their
stability has to be checked anew at every finite value of q.
|
Lines P and E in Fig. 4 were obtained for f = 0 and
comprise the well-known prolate axisymmetric shapes of free vesicles
with equatorial mirror symmetry (line P) and without such symmetry (line E), respectively. At low
a, the mirror symmetric
shapes are stable (steep, solid part of P on the left), whereas, at
point S, the mirror symmetry of stable shapes is broken. The dashed part of line P starting in S continues the sequence of now unstable mirror symmetric f = 0 shapes. The stable shapes beyond
this point are pears (line E), with the limiting shape (point L)
consisting of two different spheres connected through an infinitesimal
neck. (Note that here and in the following we use "pear" to denote
any prolate axisymmetric shape that is polar, i.e., that does not have
an equatorial reflection plane.) For q
, the shape
transition at S resembles a second-order phase transition that was
described in Svetina and
ek
(1990)
.
Because we are only interested in elongated (f
0)
axially strained vesicles, we need to inspect only the shapes located above the f = 0 lines. The upper boundary of the region
of interest (f
, line M) comprises the shapes with
the largest possible axial extension at given
a. It was
shown (Bo
i
et al., 1997
) that these limiting shapes are
mirror symmetric. Hence, there has to be a transition between mirror
symmetric elongated shapes and elongated shapes with broken mirror
symmetry. This transition takes place at the z values
forming line T. The mirror symmetric shapes located between this line
and line M are the only relevant (low-energy) solutions of the
considered variational problem in this region. Alternately, at every
point between line T and line P one finds two relevant solutions, i.e.,
a mirror symmetric stationary shape and a stationary shape with broken
mirror symmetry. In this case, the mirror symmetric shape is unstable.
This situation is illustrated in Fig. 5
showing a vertical scan through the z
a phase
diagram at
a = 1.1. It presents the local bending
energies of both solutions as a function of z and includes a
few typical shapes.
|
Shape sequences and force-extension relations at q = 4
Having mapped the stationary shapes into the above phase diagram,
we need to establish which of these shapes are successively assumed by
a real axially strained vesicle. Thus, we now consider more realistic,
finite values of the ratio q between the nonlocal and the
local bending modulus. Measured values of the nonlocal bending modulus
kr agree with estimates considering the membrane as a double layer of two homogeneous thin shells (Waugh et al., 1992
;
Raphael and Waugh, 1996
), both giving a value for
kr that is three to four times the value of the
local bending modulus kc. We choose q = 4 as a typical ratio. As explained above, within this
generalized bilayer couple model the area difference
a is a mere geometrical quantity whose value changes as the shape of a given
vesicle is deformed. In contrast, we recall that the reference value
a0 represents the difference between the
numbers of lipids constituting the two leaflets of the bilayer
membrane. Not allowing for lipid transbilayer movement (flip-flop),
a0 remains constant when an axial force
deforms the observed vesicle, and so it is this quantity that is a
basic control parameter characterizing a given vesicle.
Before turning to the shape behavior of axially strained vesicles, it
is useful to recall a well-known result of the study of free vesicles.
Comparing the stable prolate shapes obtained for q = 4
at continuously increasing values of
a0
reveals a large jump between mirror symmetric vesicle shapes and pear
shapes having an almost closed neck (Svetina and
ek
,
1992
; Miao et al., 1994
). This discontinuous (first-order) transition
is accompanied by a discontinuous change of
a at the
critical value of
a0. The intermediate
a-values correspond to unstable or metastable stationary
shapes. Hence, a number of stationary shapes of free vesicles that are
stable at q
become indeed globally unstable when
they gain the freedom to adjust
a.
We are, of course, mainly interested in the behavior of those
stationary f = 0 solutions that correspond to globally
stable shapes, i.e., to real free vesicles. When subjecting these
vesicles to an axial strain, we observe a surprising and highly
interesting variety of shape transformations. The particular shape
sequence of a strained, elongating vesicle mainly depends on the
vesicle's
a0 value. Furthermore, a given
vesicle may behave differently in the two considered experimental
scenarios (constant-z or constant-f scenario, cf.
Fig. 3). Figure 6 presents an overview of
the different types of behavior observed. It combines three typical
shape sequences obtained for representative axially strained, prolate
vesicles. The first two example vesicles (A:
a0 =
a|f=0
1.02209; and B:
a0 = 1.7,
a|f=0
1.02214) are mirror symmetric at
f = 0. As the vesicle extension increases, the mirror
symmetry is broken in both cases. In the constant-z scenario
the symmetry-breaking transition takes place along the path marked
Jz. This transition is continuous for vesicle A, whereas it
is discontinuous for vesicle B. Alternately, in the
constant-f scenario, the symmetry-breaking transition (along
path Jf) is discontinuous for both vesicles. The shapes of
the third example vesicle (C:
a0 = 1.9,
a|f=0
1.17624) are nonmirror symmetric
throughout the depicted series, and all shape changes are continuous.
|
Figure 6 only includes shapes that are globally stable in at least one
of the two possible scenarios. The computational procedure to arrive at
such shape sequences is rather lengthy. For each vesicle (i.e., for
each
a0), one first needs to find all
branches of stationary solutions that are relevant in the considered
range of the axial force f or the pole-to-pole distance
z. Figure 7 shows the
force-extension curves of stationary solutions for the three example
vesicles used in Fig. 6. The graphs clearly demonstrate that the
variety of stationary solutions is quite complex. Being able (within
the Ritz method) to analyze the stability of stationary solutions
proves to be extremely useful because it allows us, in a next step, to
focus our attention exclusively on the locally stable shapes.
Eventually, whenever two or more locally stable solutions coexist at a
given value of the control parameter (f or z),
the globally stable shape is obtained as the solution with the lowest
total energy. The interesting but somewhat technical details of this
procedure are given in the Appendix. It presents enlarged graphs of the
critical regions of Fig. 7, A and B that reveal
the (f, z) locations of shapes labeled by small letters in
Fig. 6. Furthermore, the Appendix also visualizes the deformation of
the three example vesicles by presenting the various solution branches
as trajectories in the catalog of stationary shapes that was originally
introduced in Fig. 4.
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Let us concentrate here mainly on the more practical aspects of the
force-extension relations of the three example vesicles (Figs.
7, A-C and 8). Fig. 8
continues the f-z curves of Fig. 7 for higher forces. In
these graphs, we generally use thin lines to represent the
f-z relation of axially strained, mirror symmetric stationary shapes, whereas thicker lines correspond to axially strained
pear shapes. Fig. 7, A-C reveals how the interconnection of different solution branches evolves at increasing
a0. At the largest depicted forces (upper
right regions of Fig. 7, A-C and all of Fig. 8) the
globally stable solutions are, in all three cases, the pear shapes of
the thick branch. (Note that, although at higher forces the thin branch
of mirror symmetric shapes becomes indistinguishable from the thick
pear branch, it does not merge with the latter branch but remains an
independent solution.) For the third example vesicle (Fig.
7 C) this pear branch is globally stable at all forces down
to f = 0. In contrast to that, the globally stable
solutions of the lower-force regions of Fig. 7, A and
B are the mirror symmetric shapes of the thin line (cf. also
Fig. 6). The critical region of the transition between globally stable solutions of different symmetries shifts to lower forces as we increase
a0. For more details concerning the actual
character of this transition, see the Appendix.
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It should be mentioned that new, nonmirror symmetric solutions (not
shown) continue to branch off the thin line of mirror symmetric shapes
as the force increases. The first of these additional branches appears
at f
5.03 (vesicle A), f
2.51
(vesicle B), and as low as f
1.42 for vesicle C. The corresponding transitions are in all cases continuous. As one would
expect, the stability of the mirror symmetric shapes changes at this
branching point, i.e., the mirror symmetric branch actually gains a
weak local stability. At even larger forces, the local stability of
mirror symmetric shapes alternates whenever a new nonmirror symmetric solution branch appears. Accordingly, the stability of each new, nonmirror symmetric branch is opposite from the stability of the respective mirror symmetric solution. This behavior can be easily understood and will be addressed in a later section. For now, it should
only be noted that the energy of all such branches is always
significantly higher than the energy of the coexisting, globally stable
pear branch.
A particularly interesting result is that all three vesicles behave
similarly at higher forces. The vesicles corresponding to the lines in
Fig. 8 generally have a tethered shape (cf. e.g., the last three shapes
in Fig. 6 A and C). The mirror symmetric shapes
have shorter tethers on both sides of the main vesicle body and a
reflection plane containing the equator of the main body. As mentioned
above, the force-extension curves of mirror symmetric and nonmirror
symmetric shapes become almost identical at larger forces. They are
practically indistinguishable in Fig. 8. This applies also to the
additional solution branches mentioned in the previous paragraph. Most
interestingly, in the force range depicted in Fig. 8 the unified
f-z curves become almost linear, i.e., the tethered
vesicles act as almost ideal Hookean springs. The spring constant
appears to be the same for all three vesicles, i.e., it becomes
independent of the value of
a0 in this force range. This may prove very useful for practical purposes, because
a0 is usually hard to measure experimentally.
The results of Fig. 8 suggest the system "two-point attached,
tethered vesicle" as a good candidate for an ultrasensitive spring in
micromechanical experiments. Alternately, the force needed to hold a
vesicle at a given extension clearly depends on the value of
a0, i.e., on the difference between the
numbers of lipids constituting the two membrane leaflets, and thus on
vesicle history. The tether formation from vesicles with larger
a0 values requires lower forces, which is
mainly due to the smaller nonlocal bending deformation accompanying
tether formation from vesicles with larger
a0. This feature may provide a convenient way
to measure
a0 experimentally.
In conclusion of this section, we emphasize that, beyond a certain
force, the globally stable shapes (at q = 4) are, in
all considered cases, asymmetrical. They consist of a lemon-shaped main vesicle body and a narrow membrane tether that has been pulled out
of the main body. Accordingly, we call the transitions studied above
tethering transitions. Note that the tethering transition is a
continuous shape change if the f = 0 shape of a given
vesicle is already asymmetrical. Figures 7, A-C and 8 demonstrate that large
a0 values tend to
favor the formation of a tether. Beyond the tethering transition, the
main body of a tethered vesicle becomes more spherical at increasing
pole-to-pole distances, and the tether width reduces (see Fig. 6). This
agrees well with experimental observations (cf. Figs. 1 and 2).
Phase diagrams at q = 4
The above examples provide a basic insight into the typical shape
behavior of axially strained vesicles. It is instructive to generalize
the results by extending the study to the whole range of
a0 values of prolate vesicles. Repeating the
calculations of the previous section for a large number of vesicles, we
have mapped the resulting globally stable shapes into comprehensive q = 4 phase diagrams. The natural choice of control
parameters for such diagrams is (
a0, f) in
the constant-f scenario and
(
a0, z) in the constant-z
scenario. The respective phase diagrams are shown in Fig.
9, A and B.
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In both diagrams, a given vesicle is mapped to its
a0 value on the x-axis, whereas
the vesicle's deformation due to axial strain is reflected by a
vertical upward movement in either figure. The depicted
a0 range roughly corresponds to globally
stable, prolate vesicle shapes. The thick lines (Gf in Fig.
9 A, and Gz in Fig. 9 B) divide the
region of strained vesicles into subregions of mirror and nonmirror
symmetric shapes, respectively. The globally stable mirror symmetric
shapes are confined to the lower left regions of both figures. The
diagrams confirm that at increasing deformation the globally stable
shape of every prolate vesicle will eventually be nonmirror symmetric.
Note that the global stability lines, Gf and
Gz, generally mark different shape transitions in Fig.
9, A and B (cf. the paths labeled Jf
and Jz in Fig. 6, A and B). In the
constant-f scenario (Fig. 9 A), the transition
across line Gf is everywhere discontinuous. Alternately,
line Gz in Fig. 9 B consists of two distinct
parts. To the left of the critical point Cz, line
Gz is identical with line T, marking a continuous
symmetry-breaking transition between mirror symmetric and non-mirror
symmetric globally stable shapes. To the right of point Cz,
the transition at line Gz is discontinuous. In this region,
line T (dash-dot line) merely marks the locations where
globally unstable branches of different symmetries merge. It should
briefly be mentioned that, in both scenarios, there is a small range of
a0 values where a deforming vesicle crosses the respective G line twice. In this range, the f = 0
shapes are pears. At increasing deformation, they reach a small range
of intermediate forces where their energy becomes larger than the energy of the coexisting mirror symmetric shapes. Passing the respective G line for the second time, the pear shapes become globally
stable again.
In the previous section, we have mentioned that additional nonmirror
symmetric solutions continue to appear at increasing deformation. Fig.
9, A and B include a line T' that marks the locations at which the first of these new solution branches appears in
the depicted
a0 range. For further
illustration, we have also included the (dashed) lines
Hf and Hz. These lines subdivide the region of
globally stable mirror symmetric shapes into a part where mirror
symmetric shapes are the only stationary solution (left of the
respective H line) and a part that additionally contains globally
unstable pear shapes. Furthermore, the dotted lines P and E of
stationary f = 0 solutions were included in Fig.
9 B to illustrate the locations at which various other
lines originate. The lower branches of lines P and E also represent the
lower boundary of this phase diagram.
Tether shape and degeneracy of tethered vesicles
Already, in the discussion of Figs. 7 and 8, we have noted that the force-extension curves of mirror symmetric and nonmirror symmetric shapes become almost identical at larger forces. Each of the f-z lines of the three example vesicles (A-C) shown in Fig. 8 actually represents a set of various distinct solutions, including the additional nonmirror symmetric solutions that successively appear at increasing deformation (e.g., at line T', cf. Fig. 9). Both the shapes of the latter nonmirror symmetric solutions as well as the mirror symmetric shapes have tethers on both sides of the main vesicle body. The near-identity of the f-z curves of different stationary solutions of a given vesicle strongly indicates that the tether is basically cylindrical. Obviously, we may cut off the tether on one side of the mirror symmetric shape and attach it to the tether on the other side without significantly affecting the axial force. If the tether were not cylindrical but, for example, an elongated cone, we could not do this manipulation without deforming some parts of the vesicle, which, in turn, would hardly be possible without a force change. Alternately, we found that, in all considered cases, the globally stable asymmetrical shape has a significantly lower energy than the other solutions. Furthermore, the stability analysis reveals a pronounced minimum for the globally stable asymmetrical solution, whereas the mirror symmetric solution and the additional nonmirror symmetric solutions are more or less degenerate with respect to one degree of freedom.
To resolve this puzzle, we have simulated a situation where we can push the main vesicle body along the tether while the pole-to-pole distance remains constant. This was done by introducing another constraint that enforces a fixed distance zm between the lower pole of the vesicle and the equator of the main vesicle body. Continuously changing this distance, we have monitored the resulting shapes and their elastic energy for vesicle A at z = 4.5. Energy and shapes are combined in Fig. 10. Inspecting the zm dependence of the elastic energy explains at once the degeneracy of the mirror symmetric shape and all other shapes involving two tethers. We see that we may indeed cut out a (more or less) cylindrical part of the tether on one side and add it to the tether on the other side without changing the elastic energy as long as at least a small tethered part remains on either side of the main vesicle body. Only when the tether completely disappears on one side the vesicle slides down into the energy minimum of the globally stable, asymmetrical shape. Of course, there have to be two equivalent energy minima because flipping a given shape vertically does not affect its energy. The energy difference between the minimum and the broad plateau of vesicles with two tethers can thus be ascribed to the high energy that is needed to initialize a tether, i.e., to bend the membrane into a tether right at the pole. This energy cost is paid only once if the vesicle has only one tether, which explains the global stability of the corresponding asymmetrical shape.
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These results further support that the tether shape is practically cylindrical. In contrast, if we require smoothness of the higher derivatives of the vesicle contour, it is rather unlikely that the tether is an ideal cylinder. Another indication for the existence of (small) deviations from a cylindrical tether shape is the observation that the energy plateau in Fig. 10 is not ideally flat. A small but significant energy maximum is seen adjacent to the minimum of the globally stable shape. It corresponds to that additional nonmirror symmetric stationary solution that appears first at increasing deformation (at line T' in Fig. 9). Of course, the energy plateau of Fig. 10 exhibits further minima or maxima for all other additional solutions. However, they are too weak to be recognized.
The presence of the noticeable first maximum suggests that the deviations of the tether shape from a cylinder are largest at the vesicle pole and/or the junction with the main vesicle body. To establish the importance of such deviations, we have recalculated the globally stable shape of vesicle A at z = 4.5 with very high accuracy. For this, the number of terms included in the shape expansion of the Ritz method was doubled to 200. The resulting tether shape is enlarged in Fig. 11, where the tether is somewhat distorted by the scales used for the coordinate axes. This microscopic picture of the tether contour confirms that, over most of its length, the tether is indeed indistinguishable from a cylinder. As indicated in Fig. 10 by the dependence of the elastic energy on zm, significant deviations of the tether shape from an ideal cylinder are found only at the pole and at the junction with the main body. Recent analytical results prove that these deviations act as perturbations superposing a wave-like shape with a fast decaying amplitude on the mean, cylindrical tether shape. (The details of this analysis will be published elsewhere.) For most practical purposes, however, these waves do not significantly alter the underlying cylindrical shape of the tether.
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CONCLUSIONS |
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The present theoretical paper studies the shape behavior of bilayer vesicles that are deformed by axial loads acting on two opposite points of the vesicle membrane. Restricting the calculations to prolate axisymmetric vesicle shapes, the use of general variational procedures allows us to consider arbitrary deformations and thus to overcome the limitations of parametrical models. To cover a large range of deformations, we employ or introduce mathematical methods that are particularly suitable for the description of axially strained vesicles.
Vesicles subject to low axial forces are shown to exhibit a highly
interesting and rather complex variety of elongated shapes. With the
exception of the work by Umeda et al. (1998)
, previous studies of
axially strained vesicles have been restricted exclusively to mirror
symmetric shapes (Bo
i
et al., 1997
; Kuchnir Fygenson et
al., 1997b
, where the latter work's simplifications in the physical
description of closed bilayer membranes, as well as in the parametrical
treatment, may have led to substantial uncertainties in the
quantitative predictions made). Although some of the conclusions drawn
in the very recent paper by Umeda et al. (1998)
are in agreement with
our results, that paper disregards the nonlocal bending deformation, and it also allows the vesicle volume to change (keeping the pressure difference across the membrane constant). It should be mentioned that, for the deformations considered here, mechanically induced pressure differences across the membrane are negligibly small in
comparison with pressures generated by osmotic imbalance. Therefore, because the vesicle membrane is practically impermeable to osmotically active substances over the time frame of an experiment, the vesicle volume cannot change as long as the external conditions (temperature, osmolarity) are kept constant.
The various phase diagrams (Figs. 4 and 9) presented here for prolate
vesicles with a relative volume v = 0.95 include shapes with and without equatorial mirror symmetry. Fig. 4 gives a
representative overview of the stationary shapes of axially strained
vesicles within the generalized bilayer couple model. For a
characteristic ratio, q = 4, between the nonlocal and
the local bending modulus, Fig. 9 reveals the regions of globally
stable shapes of different symmetries in dependence of the vesicle's
area difference of monolayers,
a0, and its
axial deformation. On this basis, we find that only a small fraction of
the mirror symmetric shapes studied earlier correspond to stable
solutions of the considered variational problem. Generally, the shape
behavior of axially strained vesicles is shown to be dominated by polar
shapes, i.e., by shapes with broken mirror symmetry. For q = 4, we inspect the detailed shape behavior of typical model
vesicles, and we demonstrate how additional instabilities may occur.
Higher forces are found to cause the formation of narrow tubular membrane extrusions. This tethering transition may be continuous or discontinuous. Its character depends on how the vesicle elongation is controlled (i.e., whether an increasing axial force or an increasing pole-to-pole distance is imposed), and on vesicle history (i.e.,