Keith G.
Hedlund
,
Vikina
Martinez
,
Xi
Chen
,
Cheol S.
Park
,
Joseph E.
Maclennan
*,
Matthew A.
Glaser
and
Noel A.
Clark
Department of Physics, University of Colorado, Boulder, Colorado, 80309, USA. E-mail: jem@colorado.edu
First published on 4th December 2024
We show that stable, freely suspended liquid crystal films can be made from the ferroelectric nematic (NF) phase and from the recently discovered polar, lamellar SmZA and SmAF phases. The NF films display two-dimensional, smectic-like parabolic focal conic textures comprising director/polarization bend that are a manifestation of the electrostatic suppression of director splay in the film plane. In the SmZA and SmAF phases, the smectic layers orient preferentially normal to the film surfaces, a condition never found in typical thermotropic or lyotropic lamellar LC phases, with the SmZA films exhibiting focal-conic fan textures mimicking the appearance of typical smectics in glass cells when the layers are oriented normal to the plates, and the SmAF films showing a texture of plaquettes of uniform in-plane orientation where both bend and splay are suppressed, separated by grain boundaries. The SmAF phase can also be drawn into thin filaments, in which X-ray scattering reveals that the smectic layer planes are normal to the filament axis. Remarkably, the filaments are mechanically stable even if they break, forming free-standing, fluid filaments supported only at one end. The unique architectures of these films and filaments are stabilized by the electrostatic self-interaction of the liquid crystal polarization field, which enables the formation of confined, fluid structures that are fundamentally different from those of their counterparts made using previously known liquid crystal phases.
The discovery of the NF phase stimulated a number of theoretical and simulation studies of ferroelectric and related liquid crystal polar states, many of which are summarized in recent reviews on the subject.12,13 The first atomistic simulation investigations of the molecular origins of polar order in NF materials identified a variety of characteristic molecular association motifs arising from electrostatic ‘docking’ interactions,3 a thermodynamic mechanism for polar order further explored in subsequent theoretical and simulation work.14–17 The emerging consensus is that emergent polar order involves the subtle interplay of strong electrostatic association, excluded volume interactions, and molecular conformational behavior, but predictive modeling of phase behavior in this family of materials remains an unmet challenge. The ferroelectric nematic realm has proven to be extraordinary rich, and phenomenological theories of the phases, phase transitions, and properties of these novel polar materials are under active development.12,13,18,19 Ferroelectric nematic materials have potential use in a wide range of applications, including high speed electrooptic shutters and displays, non-linear optics, fast electronic electrooptic modulators, tunable lasers, electrostatic actuators, smart windows, shutters, quantum photonic devices, energy storage, optical imaging, and sensing.20–28
Films and filaments are examples of LC preparations confined by interfacial tension at free surfaces and stabilized by LC nanostructuring. They have been found to be broadly useful in studying the effects of reduced dimensionality on liquid crystal structure and phase behavior. Single and few-layer thick freely suspended films of smectic liquid crystals, which have been studied extensively since their discovery in the 1970's,29 are confined along a single spatial dimension, yielding a unique platform for investigating two-dimensional (2D) elastohydrodynamics, interfacial effects, and phase behavior.30 The surfaces of smectic films are comprised of smectic layers, nanostructured interfaces that suppress pore formation and film rupture. Nematic LC films can be also drawn but are metastable because of their susceptibility to rupture by capillary thinning.
Freely suspended filaments can be drawn from a variety of liquid crystal systems, including discotic phases where the molecules are stacked in fluid columns aligned along the filament axis,31,32 and bent-core smectic33–36 or twist-bend phases,37 in which lamellae are arranged in concentric cylinders about the filament axis. Freely suspended filaments of nematics, and of smectics of rod-shaped molecules, tend to be very short-lived, thinning and breaking because of the Rayleigh–Plateau instability.38 However, it has recently been found that this instability can be suppressed in ferroelectric nematic filaments by applying an electric field along the filament axis. For example, in the course of exploring the use of ferroelectric nematics as thick, liquid bridges in electrostatic actuators,39 Nishimura et al. observed the transient formation of freely suspended NF filaments between planar electrodes. More recently, Máthé et al. and Jarosik et al. independently reported that the lifetime of filaments of ferroelectric nematics up to several mm in length could be extended by the appropriate application of electric fields,40,41 enabling their detailed study.
Confirmation of the smectic nature of the SmZA and SmAF phases by X-ray diffraction7,10 raised the question of whether such lamellar phases could be drawn into films or filaments that, like soap films, are “freely suspended” by their own surface tension. In this paper, we show that stable, freely suspended films can indeed be created not only in these polar smectic phases but also, remarkably, in the NF phase. In addition, we show that thin, polar filaments can be drawn in the SmAF phase, and that such filaments can be “free-standing”, i.e., mechanically stable in spite of their own surface tension. These unique characteristics arise from the dominant electrostatic self-interaction of the polarization field in these highly polar materials, which leads to film and filament structures that are fundamentally different from those of their counterparts made using previously known LC phases.
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Fig. 1 Typical polarized light microscope textures of a freely suspended 2N/DIO film in the (A) SmZA (85 °C), (B) and (C) NF (70 °C, 60 °C), and (D) SmAF (45 °C) phases, viewed in transmission. In all phases, the director and polarization are parallel to the film plane and locally have the same orientation through the film, giving dark extinction brushes between crossed polarizers. The in-plane azimuthal orientation is determined by polarization self-interactions and elasticity. Variations in birefringence color are indicative of changes in film thickness. (A) The antiferroelectric, lamellar structure of the SmZA phase leads to an irregular texture of small focal-conic fans. (B) In the NF phase, polarization splay is suppressed, leading to a bend-only texture. The central part of the image in (B) is shown in more detail in Fig. 2. (C) A large, circular NF bend domain. (D) The same area as in (C) after cooling to the SmAF phase. Here both bend and splay of the director are suppressed, leading to the formation of locally uniform, block-like smectic domains of different orientation, separated by sharp grain boundaries. Black domains are at extinction orientations. |
We now consider the origin of the preference for n being parallel to the film plane, noting that this orientation of the director is not generally found in nematic free films and has never been observed in freely suspended smectic films of calamitic or bent-core molecules, where the layers align parallel to the surfaces and the director is consequently oriented normal (or nearly normal) to the surfaces. We can model the NF film as a uniformly polarized slab with a coupled director/polarization field n(θ, φ)/P(θ, φ) making an angle θ relative to the film surface and having an orientation φ in the y, z plane of the film. Polarization self-interactions tend to suppress splay distortions of the polarization field P, so that the director/polarization field is essentially uniform through the thickness of the film.29,43–45 Tilting of such a uniform polarization block from θ = 0 would deposit space charge of magnitude Psin
θ and with opposite signs on the two film surfaces. This in turn would generate a uniform field through the thickness of the film, normal to the film plane, of magnitude E = −(P/ε)sin
θ ∼ (109 V m−1)sin
θ, the energetic cost of which effectively suppresses any deviation from planar orientation. The polarization self-interaction thus forces P to be both locally uniform through the film and parallel to the film plane, a phenomenon also observed for NF material confined in channels.18 A similar condition applies in the antiferroelectric SmZA phase, where a uniform polarization field is preferred within each smectic layer.6,7
The texture of freely suspended films in the NF phase may thus be considered to be an image of the two-dimensional director/polarization field, φ(y, z). The texture is controlled only by the LC elasticity and the self-interaction of the polarization field, which, due to polarization space charge, makes in-plane splay deformations much more energetically costly than bend. This is manifest in the films as a tiling of large areas within which n/P is uniform (blue/green regions in Fig. 2A) or is tangent to families of circles, exhibiting pure bend, with the required complementary splay being confined to narrow defect lines (polarization-stabilized kinks, curved yellow/gray lines in Fig. 1B and 2).43–45 The constraint allowing only bend of the director is the conjugate of the constraint permitting only director splay in 2D smectics,46 both of which lead to textures of 2D focal conics with characteristic defect lines in the form of parabolas or hyperbolas, as illustrated in Fig. 2. Similar free-boundary conditions are achievable in supported NF films bounded by air on top and a glycerin or untreated polymer surface on the bottom.47,48 These preparations all yield textures very similar to that shown in Fig. 1B. In contrast to conventional smectic A and C films,30 the thickness of the SmZA, NF, and SmAF films is not quantized in the sense of having a certain number of smectic layers in a given location, and the characteristic island and layer-step textures found in conventional smectic films are not observed here. Instead, as is evident from Fig. 1, the thickness of the films varies continuously across the width of the film, with the birefringence colors indicating that the films thicken significantly on approaching and entering the meniscus.
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Fig. 2 Magnified images of parabolic focal-conic line and point defects in the freely suspended 2N/DIO film in the NF phase shown in Fig. 1B. Two sets of circular contour lines, green and yellow, which the polarization/director field locally follows on opposite sides of the central parabola, are shown in (B). The parabolic focal-conic geometry guarantees that the director/polarization field, indicated schematically by colored arrows, is splay-free. |
Striking behavior related to film thickness is observed in the NF phase upon cooling, where the films thin dramatically near the point defects of the 2D focal conic texture, as illustrated in Fig. 3A. These topological defects comprise a region of circular bend of the n/P field where the director is tangent to families of concentric circles, making 2π circuits around a common center so they are strength +1 disclinations in φ(y, z). The area around the required companion −1 defects breaks up into plaquettes of uniform orientation separated by line singularities.43 As the films are cooled, local thinning around these defects leads to a mutual attraction, which causes the defects to collect spontaneously into distinct clusters. The focal conics become distorted in this process, with the parabolic defects eventually being stretched into nearly linear domain walls connecting different clusters of point defects. The film thickness d in the defect clusters of Fig. 3 is only around 100 nm, substantially thinner than the roughly 800 nm-thick, blue-green region surrounding them. The thinning is correlated with the degree of in-plane curvature of the director field, with d beginning to decrease strongly from the background film thickness on approaching the outer reaches of a defect where the circular director pattern gets established, then decreasing further on approaching the defect core, so that the films are thinnest near the defect cores, as seen in Fig. 3A. Further illustrations of defect clustering may be seen in the ESI.†
These observations suggest the following model for film thinning and defect clustering: (i) the intrinsic film stability indicates a thickness-dependent balance of disjoining pressure contributions in a film tending respectively to thin or thicken it; (ii) the defects have associated excess energy, in the form of director curvature energy/film area, Ud, and defect core energy, Vd, both of which are proportional to film thickness. These energies are reduced if the film becomes thinner, resulting in an excess contribution to the disjoining pressure that acts like a spring connecting the film surfaces, pulling them together; (iii) this tendency extends to the areas between the defects, resulting in a mutual attraction analogous to the capillary attraction of nonwetting particles on water that depresses the surface.49 (iv) this action causes the films to thin but not to the point of rupture, indicating that thinning is opposed by a repulsive pressure that increases with decreasing thickness. The origin of this pressure is not known but could originate from the film being charged relative to the surrounding bulk LC on the film holder. Such charge is expected because the meniscus at the film edge is essentially polar, varying in thickness and structure with increasing radius from the film edge to the bulk material, such that there is always some radial component of P of preferred sign, which will leave the film charged.
X-ray diffraction was carried out in transmission using a laboratory-based SAXS/WAXS system with precision beam collimation and two-dimensional image acquisition. Both SAXS and WAXS images exhibited Bragg scattering from the SmAF layering in the filaments. The SAXS images (shown in Fig. 4A and B, respectively without and with an applied longitudinal electric field) give an arc of scattering that is resolution-limited in qz at qz = qAF = 0.269 Å−1 (layer spacing dAF = 23.4 Å), comparable to the qAF = 0.267 Å−1 previously measured in the bulk SmAF phase of 2N/DIO.10 The location of the scattering arcs confirms that the smectic layer normal is generally along the filament axis, but the azimuthal scans along these arcs shown in Fig. 4C indicate a rather broad mosaic distribution of layer normals, especially in the absence of an applied electric field (cyan curve). In an applied field (green curve), this distribution narrows and evolves to show several fairly sharp, individual peaks in θ, indicating the presence of a few, well-ordered SmAF domains differing in orientation by a few degrees and filling the illuminated volume. This behavior is similar to domain patterns found in the SmAF in sandwich cells with alignment layers.10
The WAXS scans (shown in Fig. 4D) revealed, in addition to the fundamental scattering from the SmAF layering at qz = qAF, a second-order SmAF layering peak at qz = 2qAF and the fundamental scattering at qz = qCR from a crystal phase with a layer spacing at 2π/qCR ≈ 41 Å. All of these scattering features have peak intensity with q along the filament axis z, so both the SmAF and the crystal layers are oriented generally normal to the filament axis. At lower temperatures (T = 35 °C), the crystal scattering grows in intensity and the SmAF signal weakens over the course of about five minutes. As observed in SAXS, the scattering features in the WAXS scans consist of a collection of sharp sub-peaks that are distributed in azimuth. The WAXS sub-peaks also appear to be distributed in qz. However, this spreading is a geometrical artifact arising from the finite depth of the scattering volume along the X-ray beam as it passes through the diameter of the filament, giving an apparent qz that depends on position of the scattering domain along the beam. This effect is largest when the detector is close to the sample (as in WAXS), and when the sample is thick (as for filaments). The radial scan of the SAXS data in Fig. 4B shows that the X-ray scattering from the layer structure of the SmAF phase in the filaments is in fact single-peaked.
The observation that the layer normal is generally parallel to the filament surface implies that the layers are oriented normal to the surface. This is in contrast to conventional freely suspended smectic A and C films, where it is the director that is oriented preferentially normal (or nearly normal) to the film surface. In such films, the smectic layers form parallel to the film surfaces and the film thickness is quantized (an integral number of smectic layers thick). An analogous arrangement, with the layers forming parallel to the surface, is seen in bent-core liquid crystal filaments in the B7 phase. Such stacked layers are readily detected by XRD. In the case of the SmAF filaments, however, there is no evidence of such scattering, which would show up in the regions indicated by orange circles in Fig. 4D. In the SmAF phase, the dominant determinant of director orientation at the LC/air interface is the elimination of surface charge, making P and hence n orient parallel to the surface. In a filament with a cylindrical surface, this boundary condition stabilizes planar layers normal to the filament axis. We will show below that in a SmAF filament with a conical surface, this boundary condition instead stabilizes conical layers oriented normal to the surface.
Such a filament is shown in Fig. 5A, B and E where a filament initially drawn between two needles has broken and is now supported only by the left-hand needle. As the filament was drawn, it was both stabilized as a cylinder and thinned by Rayleigh–Plateau capillary forces but, in this example, these forces ultimately drove a topology-altering event, breaking the filament and leading to the formation of a hemispherical tip at the unsupported end where the Laplace pressure then acts to pump the fluid back into the filament, toward the contacting bulk material at the other end. Remarkably, broken SmAF filaments successfully resist this Laplace pressure, maintaining their extended cylindrical structure and not retracting, although they do bend downward in response to the earth's gravitational field, as seen in Fig. 5E. Images of a filament transitioning from freely suspended to free-standing after the very thin filament tethering the right-hand end breaks are shown in Fig. 5C–E. The structural stability of these free-standing filaments tethered at only one end can be understood by analogy with confined stacks of discs of uniform thickness representing the smectic layers, as illustrated in Fig. S9 (ESI†) using NECCO candy wafers and discussed further below.
Let us consider a filament with typical dimensions, radius r = 0.5 mm, and length L ∼ 10 mm. The surface tension, σ, through the Laplace pressure from the quasi-spherical end cap, compresses the smectic layering such that each layer applies a constant force 2πrσ to its neighbor along the filament axis. This compression holds the smectic layer normal parallel to the filament axis. The layers withstand the compression with only a small fractional reduction in layer spacing: −δdAF/dAF = 2σ/rB ∼ 10−4, where we have taken σ ∼ 20 erg per cm2 and B ∼ 107 erg per cm3 (the compressibility of 8CB, a typical small-molecule smectic near room temperature).52
The gravitational deformation of a broken filament such as the one depicted in Fig. 5E can be compared to beam-bending: the response of a beam with uniform mass/length clamped at one end and loaded along its length by its own weight. Downward beam deflection results from two effects:53 (i) the moment of torque transmitted along the beam, which deforms each vertical slice of the beam (each smectic layer) to be narrower at its bottom than at the top, a deformation opposed in the case of a smectic by the layer compressibility B = E, the effective Young's modulus; and (ii) shear strain Sxz, in which each vertical slice of the beam is pushed downward (along gravity) so that it slides on the neighboring material (the next smectic layer) on the side closer to the clamped end, a deformation for a solid beam that is opposed by its shear modulus G. For typical isotropic, solid beams with a length-to-width ratio L/r ∼ 10, the shear contribution is negligible, and the downward beam deflection at the end is δ ≈ (ρgAL4/8EI) ∼ 0.2 mm, where we have taken ρ = 1 g cm−3, g = 980 cm s−2, area A = πr2, and I = (2r)4/12.53
A bulk smectic is not solid but has a bulk shear modulus G = 0, with each smectic layer able to slide like a fluid sheet relative to its neighbors, a key degree of freedom of fluid smectics. In a smectic AF filament, however, such motion is prevented by the shear rigidity provided entirely by the energetics of the boundary structure at the LC/air interface, which is what keeps the layers normal to the filament axis in the first place. The surface tension σ puts the surface under extensive force along the cylinder axis, tending to keep the surface parallel to this axis. Additionally, the polarization is electrostatically constrained to be parallel to this surface, so that the fluid smectic layers orient perpendicular to the filament surfaces and terminate there. The surface tension and the electrostatics thus combine to maintain an interface that is locally smooth and locally normal to the layering plane. Shear strain Sxz would tilt P away from the filament axis (Fig. S9A, ESI†). Tilt through a small angle θ ≡ Sxz would increase the electrostatic energy per unit filament volume by Utilt = ½(P2/4ε)Sxz2,54 giving an effective shear modulus G = (P2/4ε) ∼ 109 ergs per cm2, which is sufficiently large that shear is not a factor in filament deformation by gravity as described under criterion (ii) above.
If the smectic layers at the filament surface are constrained to be normal to the surface, the local filament shape in Fig. 5 can only be cylindrical or conical, where, in the conical case, shown in Fig. 5C and G, the layering too is conical, with the layers having the same inclination Ψ as the surface, as indicated in Fig. 5F. When the filament is tethered, surface tension along the filament minimizes deviations from cylindricality, and changes in diameter along its length are effected by the alternation of conical and cylindrical segments, manifested as a series of bright and dark reflection bands as seen in Fig. 5, where the cylindrical and conical segments are outlined respectively in red and green. The boundaries between cylindrical and conical surfaces are transition regions in which the entire local smectic layering changes from conical to planar. These transitions can be quite sharp and, judging from the images of the bands, take place in the same narrow range of z across the diameter of the filament.
A ray diagram showing the geometrical optics of collecting this light, drawn for convenience in the same plane as the filament image, is shown in Fig. 5F. (In reality, this plane of reflection (x, z) is, of course, normal to the image plane (y, z), with the incident light parallel to x.) Assuming the polarization of the incident light is parallel to the filament axis, the following observations can be made: (i) Fig. 5C shows a bright line running parallel to the filament along its center (the centerline). This feature is the back-reflection from the front surface of the filament, and is observed only from places where the filament front surface is normal to the incident light. The reflection is narrowly confined to the filament center line since the filament curvature reflects other light away, and indicates that the topmost part of the filament is generally normal to the incident light in the x–z plane. (ii) Where the front surface of the filament is tilted (in the conical segments of an intact filament, for example), the reflected light (magenta rays) is deflected away from the collection aperture so that reflections from the front surface are not collected and these regions appear homogeneously dark. Regions where the filament surface is normal to the incident light, on the other hand, reflect strongly into the collection optics, giving bright bands, for example along the cylindrical segments of an intact filament, as in Fig. 5C–F. When a filament breaks at one end, the filament typically tilts down slightly in gravity, behind the plane of the image, such that the back-reflected light is no longer collected. An example is shown in Fig. 5E, where the (invisible) fine tethering filament supporting the right-hand end of the main filament has broken and the center-line feature disappears. (iii) When the tether breaks and the thick remnant filament starts slowly bending down under gravity, the bands start moving continuously and smoothly along the filament toward the free end. When the filament is sufficiently tilted, the conical regions appear bright and the cylindrical regions dark, inverting the original contrast as can be seen by comparing Fig. 5C and E, this relative brightness determined by the direction of the back reflected light. These reflections appear fuzzy because of internal optical inhomogeneity of the filament. In principle, the bright bands can be translated at will along the filament simply by changing the angle of incidence of the incident light and the location of the collection aperture. The internal textures observed in free-standing filaments are otherwise similar to those of tethered filaments.
Finally, the bright bands are clearly not homogeneous: at higher resolution (Fig. 5G), they are seen to have a texture of fuzzy, bright lines running across the filament, apparently from SmAF layering defects, which are not unusual in samples many tens of microns thick. This striated texture is similar to that found in smectics confined between flat plates where temperature change has thinned the layers, leading to chevron formation and linear walls of zig-zag defects separating domains of opposite chevron sign.55 An example of a similar texture in a cell in the smectic C phase is shown for comparison in Fig. 5G.
Freely suspended SmAF filaments were created by applying a small amount of the DIO/2N mixture in the nematic phase (at 130 °C) to the tip of a horizontal metal needle mounted inside a temperature-controlled hot stage (Instec Inc. Model HCS302) held at either 45 °C or 35 °C. The needle tip, coated with material now in the SmAF phase, is touched to a second, colinear needle mounted within the hot stage and then slowly retracted, creating a thin filament up to several cm in length stretching between the two needles. Applying a longitudinal 10 V, 2 Hz triangle-wave voltage to the filament during the drawing process greatly increased the initial stability of the filament. The electric field could be removed once the filament had been fully drawn.
The filaments were viewed in polarized reflected light on an Olympus BX51 microscope. X-ray diffraction experiments were carried out using a Forvis SAXS/WAXS diffractometer with a 30 W Xenocs Genix 3D X-ray source (Cu anode, λ = 1.54 Å) and a Dectris Eiger R 1M detector.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4cp03425b |
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