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1 \chapter{\label{chap:mc}SPONTANEOUS CORRUGATION OF DIPOLAR MEMBRANES}
2
3 \section{Introduction}
4 \label{mc:sec:Int}
5
6 The properties of polymeric membranes are known to depend sensitively
7 on the details of the internal interactions between the constituent
8 monomers. A flexible membrane will always have a competition between
9 the energy of curvature and the in-plane stretching energy and will be
10 able to buckle in certain limits of surface tension and
11 temperature.\cite{Safran94} The buckling can be non-specific and
12 centered at dislocation~\cite{Seung1988} or grain-boundary
13 defects,\cite{Carraro1993} or it can be directional and cause long
14 ``roof-tile'' or tube-like structures to appear in
15 partially-polymerized phospholipid vesicles.\cite{Mutz1991}
16
17 One would expect that anisotropic local interactions could lead to
18 interesting properties of the buckled membrane. We report here on the
19 buckling behavior of a membrane composed of harmonically-bound, but
20 freely-rotating electrostatic dipoles. The dipoles have strongly
21 anisotropic local interactions and the membrane exhibits coupling
22 between the buckling and the long-range ordering of the dipoles.
23
24 Buckling behavior in liquid crystalline and biological membranes is a
25 well-known phenomenon. Relatively pure phosphatidylcholine (PC)
26 bilayers form a corrugated or ``rippled'' phase ($P_{\beta'}$) which
27 appears as an intermediate phase between the gel ($L_\beta$) and fluid
28 ($L_{\alpha}$) phases. The $P_{\beta'}$ phase has attracted
29 substantial experimental interest over the past 30
30 years.~\cite{Sun96,Katsaras00,Copeland80,Meyer96,Kaasgaard03}, and
31 there have been a number of theoretical
32 approaches~\cite{Marder84,Carlson87,Goldstein88,McCullough90,Lubensky93,Misbah98,Heimburg00,Kubica02,Bannerjee02}
33 (and some heroic
34 simulations~\cite{Ayton02,Jiang04,Brannigan04a,deVries05,deJoannis06})
35 undertaken to try to explain this phase, but to date, none have looked
36 specifically at the contribution of the dipolar character of the lipid
37 head groups towards this corrugation. Lipid chain interdigitation
38 certainly plays a major role, and the structures of the ripple phase
39 are highly ordered. The model we investigate here lacks chain
40 interdigitation (as well as the chains themselves!) and will not be
41 detailed enough to rule in favor of (or against) any of these
42 explanations for the $P_{\beta'}$ phase.
43
44 Membranes containing electrostatic dipoles can also exhibit the
45 flexoelectric effect,\cite{Todorova2004,Harden2006,Petrov2006} which
46 is the ability of mechanical deformations to result in electrostatic
47 organization of the membrane. This phenomenon is a curvature-induced
48 membrane polarization which can lead to potential differences across a
49 membrane. Reverse flexoelectric behavior (in which applied currents
50 effect membrane curvature) has also been observed. Explanations of
51 the details of these effects have typically utilized membrane
52 polarization perpendicular to the face of the
53 membrane,\cite{Petrov2006} and the effect has been observed in both
54 biological,\cite{Raphael2000} bent-core liquid
55 crystalline,\cite{Harden2006} and polymer-dispersed liquid crystalline
56 membranes.\cite{Todorova2004}
57
58 The problem with using atomistic and even coarse-grained approaches to
59 study membrane buckling phenomena is that only a relatively small
60 number of periods of the corrugation (i.e. one or two) can be
61 realistically simulated given current technology. Also, simulations
62 of lipid bilayers are traditionally carried out with periodic boundary
63 conditions in two or three dimensions and these have the potential to
64 enhance the periodicity of the system at that wavelength. To avoid
65 this pitfall, we are using a model which allows us to have
66 sufficiently large systems so that we are not causing artificial
67 corrugation through the use of periodic boundary conditions.
68
69 The simplest dipolar membrane is one in which the dipoles are located
70 on fixed lattice sites. Ferroelectric states (with long-range dipolar
71 order) can be observed in dipolar systems with non-triangular
72 packings. However, {\em triangularly}-packed 2-D dipolar systems are
73 inherently frustrated and one would expect a dipolar-disordered phase
74 to be the lowest free energy
75 configuration.\cite{Toulouse1977,Marland1979} Dipolar lattices already
76 have rich phase behavior, but in order to allow the membrane to
77 buckle, a single degree of freedom (translation normal to the membrane
78 face) must be added to each of the dipoles. It would also be possible
79 to allow complete translational freedom. This approach
80 is similar in character to a number of elastic Ising models that have
81 been developed to explain interesting mechanical properties in
82 magnetic alloys.\cite{Renard1966,Zhu2005,Zhu2006,Jiang2006}
83
84 What we present here is an attempt to find the simplest dipolar model
85 which will exhibit buckling behavior. We are using a modified XYZ
86 lattice model; details of the model can be found in section
87 \ref{mc:sec:model}, results of Monte Carlo simulations using this model
88 are presented in section
89 \ref{mc:sec:results}, and section \ref{mc:sec:discussion} contains our conclusions.
90
91 \section{2-D Dipolar Membrane}
92 \label{mc:sec:model}
93
94 The point of developing this model was to arrive at the simplest
95 possible theoretical model which could exhibit spontaneous corrugation
96 of a two-dimensional dipolar medium. Since molecules in polymerized
97 membranes and in the $P_{\beta'}$ ripple phase have limited
98 translational freedom, we have chosen a lattice to support the dipoles
99 in the x-y plane. The lattice may be either triangular (lattice
100 constants $a/b =
101 \sqrt{3}$) or distorted. However, each dipole has 3 degrees of
102 freedom. They may move freely {\em out} of the x-y plane (along the
103 $z$ axis), and they have complete orientational freedom ($0 <= \theta
104 <= \pi$, $0 <= \phi < 2
105 \pi$). This is essentially a modified X-Y-Z model with translational
106 freedom along the z-axis.
107
108 The potential energy of the system,
109 \begin{equation}
110 \begin{split}
111 V = \sum_i &\left( \sum_{j>i} \frac{|\mu|^2}{4\pi \epsilon_0 r_{ij}^3} \left[
112 {\mathbf{\hat u}_i} \cdot {\mathbf{\hat u}_j} -
113 3({\mathbf{\hat u}_i} \cdot {\mathbf{\hat
114 r}_{ij}})({\mathbf{\hat u}_j} \cdot {\mathbf{\hat r}_{ij}})\right] \right. \\
115 & \left. + \sum_{j \in NN_i}^6 \frac{k_r}{2}\left(
116 r_{ij}-\sigma \right)^2 \right)
117 \end{split}
118 \label{mceq:pot}
119 \end{equation}
120
121 In this potential, $\mathbf{\hat u}_i$ is the unit vector pointing
122 along dipole $i$ and $\mathbf{\hat r}_{ij}$ is the unit vector
123 pointing along the inter-dipole vector $\mathbf{r}_{ij}$. The entire
124 potential is governed by three parameters, the dipolar strength
125 ($\mu$), the harmonic spring constant ($k_r$) and the preferred
126 intermolecular spacing ($\sigma$). In practice, we set the value of
127 $\sigma$ to the average inter-molecular spacing from the planar
128 lattice, yielding a potential model that has only two parameters for a
129 particular choice of lattice constants $a$ (along the $x$-axis) and
130 $b$ (along the $y$-axis). We also define a set of reduced parameters
131 based on the length scale ($\sigma$) and the energy of the harmonic
132 potential at a deformation of 2 $\sigma$ ($\epsilon = k_r \sigma^2 /
133 2$). Using these two constants, we perform our calculations using
134 reduced distances, ($r^{*} = r / \sigma$), temperatures ($T^{*} = 2
135 k_B T / k_r \sigma^2$), densities ($\rho^{*} = N \sigma^2 / L_x L_y$),
136 and dipole moments ($\mu^{*} = \mu / \sqrt{4 \pi \epsilon_0 \sigma^5
137 k_r / 2}$). It should be noted that the density ($\rho^{*}$) depends
138 only on the mean particle spacing in the $x-y$ plane; the lattice is
139 fully populated.
140
141 To investigate the phase behavior of this model, we have performed a
142 series of Metropolis Monte Carlo simulations of moderately-sized (34.3
143 $\sigma$ on a side) patches of membrane hosted on both triangular
144 ($\gamma = a/b = \sqrt{3}$) and distorted ($\gamma \neq \sqrt{3}$)
145 lattices. The linear extent of one edge of the monolayer was $20 a$
146 and the system was kept roughly square. The average distance that
147 coplanar dipoles were positioned from their six nearest neighbors was
148 1 $\sigma$ (on both triangular and distorted lattices). Typical
149 system sizes were 1360 dipoles for the triangular lattices and
150 840-2800 dipoles for the distorted lattices. Two-dimensional periodic
151 boundary conditions were used, and the cutoff for the dipole-dipole
152 interaction was set to 4.3 $\sigma$. This cutoff is roughly 2.5 times
153 the typical real-space electrostatic cutoff for molecular systems.
154 Since dipole-dipole interactions decay rapidly with distance, and
155 since the intrinsic three-dimensional periodicity of the Ewald sum can
156 give artifacts in 2-d systems, we have chosen not to use it in these
157 calculations. Although the Ewald sum has been reformulated to handle
158 2-D systems,\cite{Parry75,Parry76,Heyes77,deLeeuw79,Rhee89} these
159 methods are computationally expensive,\cite{Spohr97,Yeh99} and are not
160 necessary in this case. All parameters ($T^{*}$, $\mu^{*}$, and
161 $\gamma$) were varied systematically to study the effects of these
162 parameters on the formation of ripple-like phases.
163
164 \section{Results and Analysis}
165 \label{mc:sec:results}
166
167 \subsection{Dipolar Ordering and Coexistence Temperatures}
168 The principal method for observing the orientational ordering
169 transition in dipolar or liquid crystalline systems is the $P_2$ order
170 parameter (defined as $1.5 \times \lambda_{max}$, where
171 $\lambda_{max}$ is the largest eigenvalue of the matrix,
172 \begin{equation}
173 {\mathsf{S}} = \frac{1}{N} \sum_i \left(
174 \begin{array}{ccc}
175 u^{x}_i u^{x}_i-\frac{1}{3} & u^{x}_i u^{y}_i & u^{x}_i u^{z}_i \\
176 u^{y}_i u^{x}_i & u^{y}_i u^{y}_i -\frac{1}{3} & u^{y}_i u^{z}_i \\
177 u^{z}_i u^{x}_i & u^{z}_i u^{y}_i & u^{z}_i u^{z}_i -\frac{1}{3}
178 \end{array} \right).
179 \label{mceq:opmatrix}
180 \end{equation}
181 Here $u^{\alpha}_i$ is the $\alpha=x,y,z$ component of the unit vector
182 for dipole $i$. $P_2$ will be $1.0$ for a perfectly-ordered system
183 and near $0$ for a randomized system. Note that this order parameter
184 is {\em not} equal to the polarization of the system. For example,
185 the polarization of the perfect anti-ferroelectric system is $0$, but
186 $P_2$ for an anti-ferroelectric system is $1$. The eigenvector of
187 $\mathsf{S}$ corresponding to the largest eigenvalue is familiar as
188 the director axis, which can be used to determine a privileged dipolar
189 axis for dipole-ordered systems. The top panel in Fig. \ref{mcfig:phase}
190 shows the values of $P_2$ as a function of temperature for both
191 triangular ($\gamma = 1.732$) and distorted ($\gamma=1.875$)
192 lattices.
193
194 \begin{figure}
195 \includegraphics[width=\linewidth]{./figures/mcPhase.pdf}
196 \caption{\label{mcfig:phase} Top panel: The $P_2$ dipolar order parameter as
197 a function of temperature for both triangular ($\gamma = 1.732$) and
198 distorted ($\gamma = 1.875$) lattices. Bottom Panel: The phase
199 diagram for the dipolar membrane model. The line denotes the division
200 between the dipolar ordered (anti-ferroelectric) and disordered phases.
201 An enlarged view near the triangular lattice is shown inset.}
202 \end{figure}
203
204 There is a clear order-disorder transition in evidence from this data.
205 Both the triangular and distorted lattices have dipolar-ordered
206 low-temperature phases, and orientationally-disordered high
207 temperature phases. The coexistence temperature for the triangular
208 lattice is significantly lower than for the distorted lattices, and
209 the bulk polarization is approximately $0$ for both dipolar ordered
210 and disordered phases. This gives strong evidence that the dipolar
211 ordered phase is anti-ferroelectric. We have verified that this
212 dipolar ordering transition is not a function of system size by
213 performing identical calculations with systems twice as large. The
214 transition is equally smooth at all system sizes that were studied.
215 Additionally, we have repeated the Monte Carlo simulations over a wide
216 range of lattice ratios ($\gamma$) to generate a dipolar
217 order/disorder phase diagram. The bottom panel in Fig. \ref{mcfig:phase}
218 shows that the triangular lattice is a low-temperature cusp in the
219 $T^{*}-\gamma$ phase diagram.
220
221 This phase diagram is remarkable in that it shows an
222 anti-ferroelectric phase near $\gamma=1.732$ where one would expect
223 lattice frustration to result in disordered phases at all
224 temperatures. Observations of the configurations in this phase show
225 clearly that the system has accomplished dipolar ordering by forming
226 large ripple-like structures. We have observed anti-ferroelectric
227 ordering in all three of the equivalent directions on the triangular
228 lattice, and the dipoles have been observed to organize perpendicular
229 to the membrane normal (in the plane of the membrane). It is
230 particularly interesting to note that the ripple-like structures have
231 also been observed to propagate in the three equivalent directions on
232 the lattice, but the {\em direction of ripple propagation is always
233 perpendicular to the dipole director axis}. A snapshot of a typical
234 anti-ferroelectric rippled structure is shown in
235 Fig. \ref{mcfig:snapshot}.
236
237 \begin{figure}
238 \includegraphics[width=\linewidth]{./figures/mcSnapshot.pdf}
239 \caption{\label{mcfig:snapshot} Top and Side views of a representative
240 configuration for the dipolar ordered phase supported on the
241 triangular lattice. Note the anti-ferroelectric ordering and the long
242 wavelength buckling of the membrane. Dipolar ordering has been
243 observed in all three equivalent directions on the triangular lattice,
244 and the ripple direction is always perpendicular to the director axis
245 for the dipoles.}
246 \end{figure}
247
248 Although the snapshot in Fig. \ref{mcfig:snapshot} gives the appearance
249 of three-row stair-like structures, these appear to be transient. On
250 average, the corrugation of the membrane is a relatively smooth,
251 long-wavelength phenomenon, with occasional steep drops between
252 adjacent lines of anti-aligned dipoles.
253
254 The height-dipole correlation function ($C_{\textrm{hd}}(r, \cos
255 \theta)$) makes the connection between dipolar ordering and the wave
256 vector of the ripple even more explicit. $C_{\textrm{hd}}(r, \cos
257 \theta)$ is an angle-dependent pair distribution function. The angle
258 ($\theta$) is the angle between the intermolecular vector
259 $\vec{r}_{ij}$ and direction of dipole $i$,
260 \begin{equation}
261 C_{\textrm{hd}} = \frac{\langle \frac{1}{n(r)} \sum_{i}\sum_{j>i}
262 h_i \cdot h_j \delta(r - r_{ij}) \delta(\cos \theta_{ij} -
263 \cos \theta)\rangle} {\langle h^2 \rangle}
264 \end{equation}
265 where $\cos \theta_{ij} = \hat{\mu}_{i} \cdot \hat{r}_{ij}$ and
266 $\hat{r}_{ij} = \vec{r}_{ij} / r_{ij}$. $n(r)$ is the number of
267 dipoles found in a cylindrical shell between $r$ and $r+\delta r$ of
268 the central particle. Fig. \ref{mcfig:CrossCorrelation} shows contours
269 of this correlation function for both anti-ferroelectric, rippled
270 membranes as well as for the dipole-disordered portion of the phase
271 diagram.
272
273 \begin{figure}
274 \includegraphics[width=\linewidth]{./figures/mcHdc.pdf}
275 \caption{\label{mcfig:CrossCorrelation} Contours of the height-dipole
276 correlation function as a function of the dot product between the
277 dipole ($\hat{\mu}$) and inter-dipole separation vector ($\hat{r}$)
278 and the distance ($r$) between the dipoles. Perfect height
279 correlation (contours approaching 1) are present in the ordered phase
280 when the two dipoles are in the same head-to-tail line.
281 Anti-correlation (contours below 0) is only seen when the inter-dipole
282 vector is perpendicular to the dipoles. In the dipole-disordered
283 portion of the phase diagram, there is only weak correlation in the
284 dipole direction and this correlation decays rapidly to zero for
285 intermolecular vectors that are not dipole-aligned.}
286 \end{figure}
287
288 The height-dipole correlation function gives a map of how the topology
289 of the membrane surface varies with angular deviation around a given
290 dipole. The upper panel of Fig. \ref{mcfig:CrossCorrelation} shows that
291 in the anti-ferroelectric phase, the dipole heights are strongly
292 correlated for dipoles in head-to-tail arrangements, and this
293 correlation persists for very long distances (up to 15 $\sigma$). For
294 portions of the membrane located perpendicular to a given dipole, the
295 membrane height becomes anti-correlated at distances of 10 $\sigma$.
296 The correlation function is relatively smooth; there are no steep
297 jumps or steps, so the stair-like structures in
298 Fig. \ref{mcfig:snapshot} are indeed transient and disappear when
299 averaged over many configurations. In the dipole-disordered phase,
300 the height-dipole correlation function is relatively flat (and hovers
301 near zero). The only significant height correlations are for axial
302 dipoles at very short distances ($r \approx
303 \sigma$).
304
305 \subsection{Discriminating Ripples from Thermal Undulations}
306
307 In order to be sure that the structures we have observed are actually
308 a rippled phase and not simply thermal undulations, we have computed
309 the undulation spectrum,
310 \begin{equation}
311 h(\vec{q}) = A^{-1/2} \int d\vec{r}
312 h(\vec{r}) e^{-i \vec{q}\cdot\vec{r}}
313 \end{equation}
314 where $h(\vec{r})$ is the height of the membrane at location $\vec{r}
315 = (x,y)$.~\cite{Safran94,Seifert97} In simple (and more complicated)
316 elastic continuum models, it can shown that in the $NVT$ ensemble, the
317 absolute value of the undulation spectrum can be written,
318 \begin{equation}
319 \langle | h(q) |^2 \rangle_{NVT} = \frac{k_B T}{k_c q^4 +
320 \gamma q^2},
321 \label{mceq:fit}
322 \end{equation}
323 where $k_c$ is the bending modulus for the membrane, and $\gamma$ is
324 the mechanical surface tension.~\cite{Safran94} The systems studied in
325 this paper have essentially zero bending moduli ($k_c$) and relatively
326 large mechanical surface tensions ($\gamma$), so a much simpler form
327 can be written,
328 \begin{equation}
329 \langle | h(q) |^2 \rangle_{NVT} = \frac{k_B T}{\gamma q^2}.
330 \label{mceq:fit2}
331 \end{equation}
332
333 The undulation spectrum is computed by superimposing a rectangular
334 grid on top of the membrane, and by assigning height ($h(\vec{r})$)
335 values to the grid from the average of all dipoles that fall within a
336 given $\vec{r}+d\vec{r}$ grid area. Empty grid pixels are assigned
337 height values by interpolation from the nearest neighbor pixels. A
338 standard 2-d Fourier transform is then used to obtain $\langle |
339 h(q)|^2 \rangle$. Alternatively, since the dipoles sit on a Bravais
340 lattice, one could use the heights of the lattice points themselves as
341 the grid for the Fourier transform (without interpolating to a square
342 grid). However, if lateral translational freedom is added to this
343 model (a likely extension), an interpolated grid method for computing
344 undulation spectra will be required.
345
346 As mentioned above, the best fits to our undulation spectra are
347 obtained by setting the value of $k_c$ to 0. In Fig. \ref{mcfig:fit} we
348 show typical undulation spectra for two different regions of the phase
349 diagram along with their fits from the Landau free energy approach
350 (Eq. \ref{mceq:fit2}). In the high-temperature disordered phase, the
351 Landau fits can be nearly perfect, and from these fits we can estimate
352 the tension in the surface. In reduced units, typical values of
353 $\gamma^{*} = \gamma / \epsilon = 2500$ are obtained for the
354 disordered phase ($\gamma^{*} = 2551.7$ in the top panel of
355 Fig. \ref{mcfig:fit}).
356
357 Typical values of $\gamma^{*}$ in the dipolar-ordered phase are much
358 higher than in the dipolar-disordered phase ($\gamma^{*} = 73,538$ in
359 the lower panel of Fig. \ref{mcfig:fit}). For the dipolar-ordered
360 triangular lattice near the coexistence temperature, we also observe
361 long wavelength undulations that are far outliers to the fits. That
362 is, the Landau free energy fits are well within error bars for most of
363 the other points, but can be off by {\em orders of magnitude} for a
364 few low frequency components.
365
366 We interpret these outliers as evidence that these low frequency modes
367 are {\em non-thermal undulations}. We take this as evidence that we
368 are actually seeing a rippled phase developing in this model system.
369
370 \begin{figure}
371 \includegraphics[width=\linewidth]{./figures/mcLogFit.pdf}
372 \caption{\label{mcfig:fit} Evidence that the observed ripples are {\em
373 not} thermal undulations is obtained from the 2-d Fourier transform
374 $\langle |h^{*}(\vec{q})|^2 \rangle$ of the height profile ($\langle
375 h^{*}(x,y) \rangle$). Rippled samples show low-wavelength peaks that
376 are outliers on the Landau free energy fits by an order of magnitude.
377 Samples exhibiting only thermal undulations fit Eq. \ref{mceq:fit}
378 remarkably well.}
379 \end{figure}
380
381 \subsection{Effects of Potential Parameters on Amplitude and Wavelength}
382
383 We have used two different methods to estimate the amplitude and
384 periodicity of the ripples. The first method requires projection of
385 the ripples onto a one dimensional rippling axis. Since the rippling
386 is always perpendicular to the dipole director axis, we can define a
387 ripple vector as follows. The largest eigenvector, $s_1$, of the
388 $\mathsf{S}$ matrix in Eq. \ref{mceq:opmatrix} is projected onto a
389 planar director axis,
390 \begin{equation}
391 \vec{d} = \left(\begin{array}{c}
392 \vec{s}_1 \cdot \hat{i} \\
393 \vec{s}_1 \cdot \hat{j} \\
394 0
395 \end{array} \right).
396 \end{equation}
397 ($\hat{i}$, $\hat{j}$ and $\hat{k}$ are unit vectors along the $x$,
398 $y$, and $z$ axes, respectively.) The rippling axis is in the plane of
399 the membrane and is perpendicular to the planar director axis,
400 \begin{equation}
401 \vec{q}_{\mathrm{rip}} = \vec{d} \times \hat{k}
402 \end{equation}
403 We can then find the height profile of the membrane along the ripple
404 axis by projecting heights of the dipoles to obtain a one-dimensional
405 height profile, $h(q_{\mathrm{rip}})$. Ripple wavelengths can be
406 estimated from the largest non-thermal low-frequency component in the
407 Fourier transform of $h(q_{\mathrm{rip}})$. Amplitudes can be
408 estimated by measuring peak-to-trough distances in
409 $h(q_{\mathrm{rip}})$ itself.
410
411 A second, more accurate, and simpler method for estimating ripple
412 shape is to extract the wavelength and height information directly
413 from the largest non-thermal peak in the undulation spectrum. For
414 large-amplitude ripples, the two methods give similar results. The
415 one-dimensional projection method is more prone to noise (particularly
416 in the amplitude estimates for the distorted lattices). We report
417 amplitudes and wavelengths taken directly from the undulation spectrum
418 below.
419
420 In the triangular lattice ($\gamma = \sqrt{3}$), the rippling is
421 observed for temperatures ($T^{*}$) from $61-122$. The wavelength of
422 the ripples is remarkably stable at 21.4~$\sigma$ for all but the
423 temperatures closest to the order-disorder transition. At $T^{*} =
424 122$, the wavelength drops to 17.1~$\sigma$.
425
426 The dependence of the amplitude on temperature is shown in the top
427 panel of Fig. \ref{mcfig:Amplitude}. The rippled structures shrink
428 smoothly as the temperature rises towards the order-disorder
429 transition. The wavelengths and amplitudes we observe are
430 surprisingly close to the $\Lambda / 2$ phase observed by Kaasgaard
431 {\it et al.} in their work on PC-based lipids.\cite{Kaasgaard03}
432 However, this is coincidental agreement based on a choice of 7~\AA~as
433 the mean spacing between lipids.
434
435 \begin{figure}
436 \includegraphics[width=\linewidth]{./figures/mcProperties_sq.pdf}
437 \caption{\label{mcfig:Amplitude} a) The amplitude $A^{*}$ of the ripples
438 vs. temperature for a triangular lattice. b) The amplitude $A^{*}$ of
439 the ripples vs. dipole strength ($\mu^{*}$) for both the triangular
440 lattice (circles) and distorted lattice (squares). The reduced
441 temperatures were kept fixed at $T^{*} = 94$ for the triangular
442 lattice and $T^{*} = 106$ for the distorted lattice (approximately 2/3
443 of the order-disorder transition temperature for each lattice).}
444 \end{figure}
445
446 The ripples can be made to disappear by increasing the internal
447 elastic tension (i.e. by increasing $k_r$ or equivalently, reducing
448 the dipole moment). The amplitude of the ripples depends critically
449 on the strength of the dipole moments ($\mu^{*}$) in Eq. \ref{mceq:pot}.
450 If the dipoles are weakened substantially (below $\mu^{*}$ = 20) at a
451 fixed temperature of 94, the membrane loses dipolar ordering
452 and the ripple structures. The ripples reach a peak amplitude of
453 3.7~$\sigma$ at a dipolar strength of 25. We show the dependence
454 of ripple amplitude on the dipolar strength in
455 Fig. \ref{mcfig:Amplitude}.
456
457 \subsection{Distorted lattices}
458
459 We have also investigated the effect of the lattice geometry by
460 changing the ratio of lattice constants ($\gamma$) while keeping the
461 average nearest-neighbor spacing constant. The anti-ferroelectric state
462 is accessible for all $\gamma$ values we have used, although the
463 distorted triangular lattices prefer a particular director axis due to
464 the anisotropy of the lattice.
465
466 Our observation of rippling behavior was not limited to the triangular
467 lattices. In distorted lattices the anti-ferroelectric phase can
468 develop nearly instantaneously in the Monte Carlo simulations, and
469 these dipolar-ordered phases tend to be remarkably flat. Whenever
470 rippling has been observed in these distorted lattices
471 (e.g. $\gamma = 1.875$), we see relatively short ripple wavelengths
472 (14 $\sigma$) and amplitudes of 2.4~$\sigma$. These ripples are
473 weakly dependent on dipolar strength (see Fig. \ref{mcfig:Amplitude}),
474 although below a dipolar strength of $\mu^{*} = 20$, the membrane
475 loses dipolar ordering and displays only thermal undulations.
476
477 The ripple phase does {\em not} appear at all values of $\gamma$. We
478 have only observed non-thermal undulations in the range $1.625 <
479 \gamma < 1.875$. Outside this range, the order-disorder transition in
480 the dipoles remains, but the ordered dipolar phase has only thermal
481 undulations. This is one of our strongest pieces of evidence that
482 rippling is a symmetry-breaking phenomenon for triangular and
483 nearly-triangular lattices.
484
485 \subsection{Effects of System Size}
486 To evaluate the effect of finite system size, we have performed a
487 series of simulations on the triangular lattice at a reduced
488 temperature of 122, which is just below the order-disorder transition
489 temperature ($T^{*} = 139$). These conditions are in the
490 dipole-ordered and rippled portion of the phase diagram. These are
491 also the conditions that should be most susceptible to system size
492 effects.
493
494 \begin{figure}
495 \includegraphics[width=\linewidth]{./figures/mcSystemSize.pdf}
496 \caption{\label{mcfig:systemsize} The ripple wavelength (top) and
497 amplitude (bottom) as a function of system size for a triangular
498 lattice ($\gamma=1.732$) at $T^{*} = 122$.}
499 \end{figure}
500
501 There is substantial dependence on system size for small (less than
502 29~$\sigma$) periodic boxes. Notably, there are resonances apparent
503 in the ripple amplitudes at box lengths of 17.3 and 29.5 $\sigma$.
504 For larger systems, the behavior of the ripples appears to have
505 stabilized and is on a trend to slightly smaller amplitudes (and
506 slightly longer wavelengths) than were observed from the 34.3 $\sigma$
507 box sizes that were used for most of the calculations.
508
509 It is interesting to note that system sizes which are multiples of the
510 default ripple wavelength can enhance the amplitude of the observed
511 ripples, but appears to have only a minor effect on the observed
512 wavelength. It would, of course, be better to use system sizes that
513 were many multiples of the ripple wavelength to be sure that the
514 periodic box is not driving the phenomenon, but at the largest system
515 size studied (70 $\sigma$ $\times$ 70 $\sigma$), the number of dipoles
516 (5440) made long Monte Carlo simulations prohibitively expensive.
517
518 \section{Discussion}
519 \label{mc:sec:discussion}
520
521 We have been able to show that a simple dipolar lattice model which
522 contains only molecular packing (from the lattice), anisotropy (in the
523 form of electrostatic dipoles) and a weak elastic tension (in the form
524 of a nearest-neighbor harmonic potential) is capable of exhibiting
525 stable long-wavelength non-thermal surface corrugations. The best
526 explanation for this behavior is that the ability of the dipoles to
527 translate out of the plane of the membrane is enough to break the
528 symmetry of the triangular lattice and allow the energetic benefit
529 from the formation of a bulk anti-ferroelectric phase. Were the weak
530 elastic tension absent from our model, it would be possible for the
531 entire lattice to ``tilt'' using $z$-translation. Tilting the lattice
532 in this way would yield an effectively non-triangular lattice which
533 would avoid dipolar frustration altogether. With the elastic tension
534 in place, bulk tilt causes a large strain, and the least costly way to
535 release this strain is between two rows of anti-aligned dipoles.
536 These ``breaks'' will result in rippled or sawtooth patterns in the
537 membrane, and allow small stripes of membrane to form
538 anti-ferroelectric regions that are tilted relative to the averaged
539 membrane normal.
540
541 Although the dipole-dipole interaction is the major driving force for
542 the long range orientational ordered state, the formation of the
543 stable, smooth ripples is a result of the competition between the
544 elastic tension and the dipole-dipole interactions. This statement is
545 supported by the variation in $\mu^{*}$. Substantially weaker dipoles
546 relative to the surface tension can cause the corrugated phase to
547 disappear.
548
549 The packing of the dipoles into a nearly-triangular lattice is clearly
550 an important piece of the puzzle. The dipolar head groups of lipid
551 molecules are sterically (as well as electrostatically) anisotropic,
552 and would not pack in triangular arrangements without the steric
553 interference of adjacent molecular bodies. Since we only see rippled
554 phases in the neighborhood of $\gamma=\sqrt{3}$, this implies that
555 even if this dipolar mechanism is the correct explanation for the
556 ripple phase in realistic bilayers, there would still be a role played
557 by the lipid chains in the in-plane organization of the triangularly
558 ordered phases which could support ripples. The present model is
559 certainly not detailed enough to answer exactly what drives the
560 formation of the $P_{\beta'}$ phase in real lipids, but suggests some
561 avenues for further experiments.
562
563 The most important prediction we can make using the results from this
564 simple model is that if dipolar ordering is driving the surface
565 corrugation, the wave vectors for the ripples should always found to
566 be {\it perpendicular} to the dipole director axis. This prediction
567 should suggest experimental designs which test whether this is really
568 true in the phosphatidylcholine $P_{\beta'}$ phases. The dipole
569 director axis should also be easily computable for the all-atom and
570 coarse-grained simulations that have been published in the literature.
571
572 Our other observation about the ripple and dipolar directionality is
573 that the dipole director axis can be found to be parallel to any of
574 the three equivalent lattice vectors in the triangular lattice.
575 Defects in the ordering of the dipoles can cause the dipole director
576 (and consequently the surface corrugation) of small regions to be
577 rotated relative to each other by 120$^{\circ}$. This is a similar
578 behavior to the domain rotation seen in the AFM studies of Kaasgaard
579 {\it et al.}\cite{Kaasgaard03}
580
581 Although our model is simple, it exhibits some rich and unexpected
582 behaviors. It would clearly be a closer approximation to the reality
583 if we allowed greater translational freedom to the dipoles and
584 replaced the somewhat artificial lattice packing and the harmonic
585 elastic tension with more realistic molecular modeling potentials.
586 What we have done is to present a simple model which exhibits bulk
587 non-thermal corrugation, and our explanation of this rippling
588 phenomenon will help us design more accurate molecular models for
589 corrugated membranes and experiments to test whether rippling is
590 dipole-driven or not.