• Aucun résultat trouvé

Frustration and helicity in the ordered phases of a discotic compound

N/A
N/A
Protected

Academic year: 2021

Partager "Frustration and helicity in the ordered phases of a discotic compound"

Copied!
24
0
0

Texte intégral

(1)

HAL Id: jpa-00210929

https://hal.archives-ouvertes.fr/jpa-00210929

Submitted on 1 Jan 1989

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.

Frustration and helicity in the ordered phases of a discotic compound

Paul A. Heiney, Ernest Fontes, Wim H. de Jeu, Antoni Riera, Patrick Carroll, Amos B. Smith

To cite this version:

Paul A. Heiney, Ernest Fontes, Wim H. de Jeu, Antoni Riera, Patrick Carroll, et al.. Frustration and helicity in the ordered phases of a discotic compound. Journal de Physique, 1989, 50 (4), pp.461-483.

�10.1051/jphys:01989005004046100�. �jpa-00210929�

(2)

Frustration and helicity in the ordered phases of a discotic compound

Paul A. Heiney (1), Ernest Fontes (1), Wim H. de Jeu (2,*) , Antoni Riera (3),

Patrick Carroll (3) and Amos B. Smith, III (3)

(1) Department of Physics and Laboratory for Research on the Structure of Matter, University of Pennsylvania, Philadelphia, PA 19104, U.S.A.

(2) FOM-Institute for Atomic and Molecular Physics, Kruislaan 407, 1098 SJ Amsterdam, The Netherlands

(3) Department of Chemistry and Laboratory for Research on the Structure of Matter, University of Pennsylvania, Philadelphia, PA 19104, U. S . A.

(Reçu le 6 septembre 1988, accepté le 17 octobre 1988)

Resume.

2014

Nous avons étudié les mesophases Dhd et Dho et la phase cristalline K à basse

température de l’hexa(hexylthio)triphenylene par diffraction de rayons X. La phase cristal liquide Dhd à haute température est formée d’un arrangement triangulaire à deux dimensions de colonnes

avec un ordre entre colonnes à courte distance. La phase Dho à température intermédiaire est formée d’un arrangement triangulaire de colonnes ayant un ordre périodique de position et un

ordre hélicoïdal incommensurable. En outre, on retrouve un super-réseau à trois colonnes qui peut résulter de la frustration imposée par l’interdigitation de la symétrie triangulaire. Nous suggérons que la transition Dhd ~ Dho. est déterminée par l’augmentation de rigidité et de longueur des chaînes hydrocarbonées due à la décroissance en température. La phase K est monoclinique. La transition K ~ Dho peut s’effectuer par un déplacement moléculaire relative- ment petit.

Abstract.

2014

We have used X-ray diffraction to study the discotic mesophases Dhd and Dho and the low temperature crystalline K phase of hexa(hexylthio)triphenylene. The high- temperature liquid crystalline Dhd phase is composed of a two-dimensional triangular array of columns, with short range intracolumn order. The intermediate-temperature Dho phase consists of

a triangular array of columns with periodic positional and incommensurate helical intracolumn order. Furthermore, a three-column superlattice is found, which may result from the frustration

imposed by molecular interdigitation in triangular symmetry. We suggest that the Dhd ~ Dho transition is driven by the increase in hydrocarbon tail stiffness and length with decreasing

temperature. The K phase is found to be monoclinic. The K ~ Dho transition can be accomplished by a relatively minor displacement of the molecules.

Classification

Physics Abstracts

64.70Md - 61.30Eb

-

61.65 + d

(*) Also at the Open University, P.O. Box 2690, 6401 DL Heerlen, The Netherlands.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01989005004046100

(3)

1. Introduction.

Liquid crystals [1] have provided us with interesting structures in which ordering takes place

in less than three dimensions, and thus are unique model systems to study low-dimensional

phase transitions [2]. Conventional rod-like mesogens may form a nematic phase, with short- range positional and long-range orientational order, or various types of smectic phase, which

have in common a well-defined density modulation in one dimension. The simplest type of smectic phase is smectic-A which has liquid-like order in the other two dimensions. Discotic

liquid crystals [3] are composed of disc-shaped niolecules with rigid planar central cores and typically 6-8 flexible hydrocarbon chain tails. They form nematic phases, and also more highly

ordered columnar mesophases consisting of two-dimensional arrays of columns.

Columnar discotic phases have been classified according to the symmetry of the columns and the nature of the intracolumn order. The most commonly observed « hexagonal

disordered » Dhd phase consists of a triangular array of columns with only fluid-like

intracolumn order and consequently no long-range column-column correlation of the molecular heights. In cases where the molecules are tilted with respect to the long axis of the column, or where the 3-fold molecular symmetry is broken, a « rectangular disordered » Drd phase can also be found [4, 5]. Additionally, the molecules within each column may order to form the hexagonal ordered phase Dho. However, if true long-range intracolumn order

develops then the columns must be correlated, since long-range order in one dimension is not

possible. Ordered columnar phases may thus be analogs of higher smectic phases [6], which

are three-dimensional crystals with local structures close to those of true smectic phases.

There are theoretical indications [7, 8] that the phase transition from the crystalline phase to

the Dhd phase may be second order ; however, this transition has not been studied

experimentally.

In this paper we present X-ray results in a single-crystal geometry of the various phases of hexa(hexylthio)triphenylene [9] (HHTT, Fig. la). This discotic mesogen is unique in having

both a Dho and a Dhd phase at temperatures intermediate between those of the crystalline (K)

and isotropic (I) phases [10]. As far as we are aware this is the first example of a order-

disorder transition within the columns retaining the hexagonal columnar lattice intact. In other materials such a transition is usually accompanied by a change from a hexagonal to a rectangular lattice. Preliminary results on the Dhd-Dho phase transition have already been given elsewhere [10, 11]. In the Dho phase helical order develops within the columns,

associated with the molecular orientations. The helical period is incommensurate with the intermolecular spacing. Additionally, a three-column superlattice develops, associated with both the helical phase and the vertical displacement of the three columns. A model will be

presented in which this structure is a solution to the frustration imposed by both molecular

interdigitation and rotational degrees of freedom in a triangular lattice. The Dhd phase shows

an unusual negative thermal expansion coefficient, which is most likely associated with

stiffening of the aliphatic tails of the molecules.

Though the crystal structures of several mesogenic compounds have been determined [12],

it has not been possible to establish general rules relating the structure of the crystalline phase

to that of the mesophase that occurs upon melting. In many cases a considerable enthalpy change is associated with the first phase transition upon heating from the crystalline phase.

This indicates important structural relaxations, and consequently little correspondence

between the structures of the two phases can be expected. The situation may be different

when the transition from the crystal to the isotropic liquid goes in a series of steps with

enthalpy changes of the same order of magnitude. For rod-like molecules this is the case when

several higher-ordered smectics occur, and similarly with disk-like molecules when the

(4)

Fig. 1.

-

(a) Hexa(hexylthio)triphenylene (HHTT) ; (b) the pin is drawn slowly from the bulk material in the cup to produce a freely-suspended strand ; (c) the strand fixed axes and reciprocal lattice

are defined with the column axis parallel to 6z and Qx along the (100) direction. With scattering vector q

defined, ~ and X are used as azimuthal and polar angles, respectively.

transitions involve several columnar phases. The K phase in the present compound turns out

to have a monoclinic structure, but with a fundamental spacing that equals that in the

Dho phase. Hence, the K-Dho transition can be accomplished by a relatively small displacement of the molecules.

The plan of the paper is as follows. In section 2 the experimental methods are discussed, including some details of growing and characterizing discotic strands in the Dhd and Dho phases. Section 3 gives the X-ray results for the Dhd and Dho phases and a qualitative

discussion of the structures and the phase transition. Section 4 contains the structure determination of the K phase. Using these ingredients in section 5 a model for the

Dho phase is developed, followed by a brief discussion in section 6.

2. Experimental.

The HHTT sample was synthesized by Kohne et al. as described elsewhere [9], and was found

to give the following phase sequence :

Freely-suspended columnar phase strands with a single-crystal geometry were studied using a high-resolution 4-circle X-ray diffractometer. As discussed below, a sharp and well-

characterized instrumental resolution function and a well characterized and oriented strand

(5)

permitted detailed analysis of the intrinsic peak positions and lineshapes. However, the anisotropic sample mosaic introduced uncertainties in the integrated peak intensities, and

thus into the detailed analysis of the molecular conformations. Due to extreme supercooling,

the evolution of the Dho phase was observed on cooling to well below 62 °C, and details of the

Dho H K phase transition could not be studied. The unit cell structure of the K phase was

determined from a single-crystal sample using an Enraf-Nonius CAD4 diffractometer. This

technique is inappropriate for detailed lineshape measurements, but yields reliable integrated peak intensities for structural refinement.

Freely-suspended strands of the Dhd and Dho phases were obtained using a technique first developed by Safinya et al. [5]. They were grown in situ in a two-stage temperature controlled

oven [13]. Pictured schematically in figure lb, as a pin was inserted and then slowly (1 Um/min) pulled out of a cup reservoir, a fiber or strand of approximately 150-200 >m in diameter was drawn to a length of 1.5-2 mm. Retractable periscopes provided a microscopic

view of the strand during its growth ; the best quality strands were uniform in thickness and

optical clarity, while poor ones had opaque bulk-like regions. Strands were grown and annealed for 12-24 h at high temperatures in the Dhd phase. Good quality strands could not be drawn in the Dho phase, and strands in the nematic and isotropic phases were not self- supporting. The column axes were approximately oriented along the direction of the strand

pull, referred to as the strand z-axis. The orthogonal x-y plane is the plane of hexagonal symmetry of the column packing, and is referred to as the hexagonal basal plane. The reciprocal space basis is labeled Qx, Qy, and Qz ; Qb refers to an arbitrary direction in the

hexagonal basal plane. qx, qy, qz and qb refer to measured diffraction components in the above directions (Fig. lc). In the discussion that follows below we will use a triangular reciprocal

lattice to describe the Dhd and Dho phases : H and K are triangular Bragg indices in the basal

plane (qx is oriented along the (H00 ) direction) and L is the index describing reflections oriented along the column axis.

The temperature controlled sample oven was accurately positioned to within 10 >m of the center of a Huber 4-circle diffractometer. The X-ray windows defining the temperature stages

were thin-walled beryllium cylinders coaxial with the oven long axis. The outermost window

provided a sealed barrier against external thermal fluctuations and convection. The two internal windows were integral components of two concentric heating stages ; the inner stage

was controlled at the desired sample temperature, and the second stage was held 1 °C lower.

The temperature uniformity over the strand sample was balanced to better than 0.01 °C. A helium atmosphere was maintained inside the oven. The total attenuation of the X-ray beam

due to the windows was 35 %.

An Elliott GX-13 rotating anode generator with a fine-focus source diameter of 100 I£m was

employed to collect the X-ray data on the Dhd and Dho - phase strands. A vertical focussing LiF(200) monochromator crystal provided an incident flux of approximately 107 CuKal photons/second into a 400 )JLm diameter circular spot at the sample position. Using a flat LiF(200) analysing crystal this configuration yielded an in-plane longitudinal resolution of

AI q 1 =0.005Â’ full width at half maximum (FWHM), and an in-plane transverse

resolution of àq, = 0.0007 Â- 1 FWHM. The vertical resolution was determined by slits placed after the monochromator and before the scintillation detector, adjusted such that the vertical angular convergence of the incident X-ray beam onto the sample matched the vertical

angular acceptance of the detector. Two slit configurations were used, yielding for low

vertical resolution Aq,,,,

=

0.27 -1, and for high vertical resolution qvert

=

0.027 -1. In the high vertical resolution mode, the total incident flux onto the sample was reduced by a

factor of ten.

The instrumental longitudinal and transverse resolution were modeled in our data analysis

(6)

by Gaussian lineshapes with widths corresponding to àqll and Aq, . The vertical resolution

was triangular with an acceptance range of àqve,, as determined by the convolution of two square slit functions. In addition to instrumental broadening, the Bragg peaks were

broadened by intrinsic sample mosaic. There were two possible sources of this broadening : (1) from a multicrystalline sample, the measured profiles are the sum of the intensity scattered by all domains in the region of the strand illuminated by the incident X-ray beam ; (2) in a single-crystal sample, broadening may result from strain fields inside the strand. Experimen- tally, the broadening was described by two mosaic widths. The polar misalignment of the z-

axis of the strand could be described by a Gaussian distribution in polar angle with width of about 2. 2° . The azimuthal rotational distribution about the strand long axis was typically 1.5-

2°. As a result, in our analysis the intrinsic sample scattering was modelled by a three-

dimensional Gaussian ellipsoid of revolution.

The diffracted intensity was quite sensitive to both the position and the alignment of the

strand in the beam. The alignment of the strand (i.e. the orientation of the reciprocal space

axes) was determined by measuring the positions of the six primary (100) triangular peaks at regular intervals during an experiment. Likewise, the translational displacement of the strand

was calculated and corrected by comparing the intensities of these six peaks. (Since the absorption of the X-ray beam by the sample was quite small, measurement of the beam attenuation by the sample was insufficient to accurately position the strand). Through an

iterative process the strand could ultimately be centered in the beam to within 20 itm and its orientation determined to within 0.1 ° .

The sample mosaic, strand position, X-ray spot-size and instrumental resolution coupled in

a complicated way, resulting in systematic variations in measured intensity that were

unrelated to the intrinsic scattering amplitude. For structural determinations, the quantity of

interest is the integrated intensity under each Bragg peak. Peak intensities (which are listed in

Tab. 1 for the Dho phase) were measured by two methods : 1) Strong peaks were characterized

by diffraction profiles measured in three orthogonal directions, and 2) the intensities of weak

peaks were determined by carefully measuring (i.e. counting for relatively long time periods)

the scattering at the indexed Bragg position. In the second case, the integrated intensities

were calculated from peak intensities using an analytic form derived from the convolution of the instrumental resolution with the sample mosaic. We estimate the overall uncertainty in

our peak intensities to be ± 10-30 % for the strongest peaks and ± 0.5 (counts/s) for the

weakest peaks. Nevertheless, since the peak intensities spanned a dynamic range of about

104, we can say a great deal about the structure of the Dhd and Dho phases, as will be discussed

in detail later on. The effect of strand misorientation on peak positions was minimized by

careful measurements of vector differences between peaks ; we estimate our overall precision

in peak position at AI q 1 _«- 1.0 x 10- 3 A-1.

The effects of instrumental resolution and sample mosaic on X-ray peak profiles are

illustrated in figure 2. Figure 2a shows equal intensity contours of a peak in the

qx - qz plane. The long axis of the rod-shaped contours results from the convolution of the instrumental vertical resolution with the polar mosaic, while the short axis results from the instrumental longitudinal resolution. For example, the long axis dimension àq

=

0.047 A-1

FWHM results from the sum in quadrature of the vertical resolution width Oq,,ert

=

0.027 Â -1 1 FWHM and the polar mosaic width

Figure 2b shows an equal intensity contour plot of raw scattering data collected in the qZ

=

1.727 Â -1 1 plane (L

=

1). The lineshapes of peaks in this plane are determined by the

convolution of the vertical resolution function and mosaic broadening. In this sample the

(7)

Table 1.

-

Measured intensities (with estimated uncertainties) in counts per second, and calculated intensities for Bragg peaks in the Dho phase. Measured integrated intensities are

derived from either peak intensities or orthogonal scans through Bragg peaks, as discussed in text. Calculated intensities are the result of a best fit to model III with adjustable parameters

given in table II.

strand axis was misoriented from the oven long axis by a polar rotation of 1.75° about the

[1, 1, 0] crystal direction, and was additionally broadened in this direction by approximately

2. 2° . Thus, the polar profiles of nominally equivalent peaks vary somewhat : for instance, the peaks along the [x, x, 1 ] line are broadened in the orthogonal direction by both mosaic and the instrumental resolution.

The structure of the K phase was determined using a single crystal 0.04 x 0.15 x

0.05 mm3 sample which was recrystallized from hexane. The crystal was mounted on an

Enraf-Nonius CAD4 automated diffractometer and studied with Ni-filtered CuKa radiation.

A total of 5 280 reflections were measured by the w - 2 () scan technique, of which 2 656 with

intensity 1 > 3 were used in the structure solution and refinement.

(8)

Fig. 2. - (a) Equal intensity contour plot of X-ray scattering data collected in the 6z - Qx plane about

the (2, 0, 0.379) peak position ; (b) equal intensity contour plot of X-ray scattering data collected in the q2

=

1.727 A -1 1 plane (L

=

1 ). The (001), (101) and (011) peak positions, and the line [x, x, 1 ], are

indicated. Contours are drawn at values of 4 642, 3 167, 2 154, 1 602, 1 000, 681, 464, 317, 215, 160, 100 and 68 counts/30 s. The six peaks with 1 1 1 ( 33 symmetry have approximately equal intensity maxima

of 5 800 counts/30 s. Data are missing from the lower left quadrant due to a mechanical limitation of the diffractometer.

3. Columnar phases.

The diffraction patterns observed in the Dhd and Dho phases are summarized in figure 3. In the Dhd phase only the reflections corresponding to the solid circles are found. The diffraction pattern in this phase is very similar to that previously observed in a hexa-substituted truxene mesogen [13]. In the equatorial plane, a triangular array of sharp (HKO )-type reflections is

observed, corresponding to long-range (correlation length 03BE > 800 À) hexagonal ordering of

the columns. A single diffuse meridional (001) peak at qz = 1.727 Â- 1 is due to intracolumn

liquid-like ordering of the disks. The correlation length along the columns grows upon cooling from e

=

16 A at 89 °C to e

=

30 A at 76 °C, corresponding to from 4 to 8 stacked molecules.

In the transverse directions, the (001) peak is diffuse over a spherical shell with polar width of approximately 35° FWHM. Additional diffuse scattering due to the hydrocarbon tails is

centered 45° off the q, axis at a momentum transfer magnitude of 1.3 -1 ; it can be

empirically described by a functional form

(9)

Fig. 3.

-

Perspective schematic of diffraction pattern. qx and qz indicate equatorial and meridional components of the scattering vector, as discussed in text. Circle radii are proportional to the log of the peak intensity ; we measured 14 700 counts/s and 1.7 counts/s in the (100) and (300) peaks, respectively.

Open circles indicate peaks observed in the Dho phase only ; solid circles those found in both

D ho and D hd phases.

Such diffuse off-axis scattering has been previously observed in discotic mesophases [14], and

may arise either from a preferred tendency of the tails to tilt up or down, resulting in an

oriented tail-tail correlation function, or from short-range helical positional order. In any case, the diffuse scattering is most likely primarily due to the aliphatic tails, and corresponds

to a liquid-like mean tail-tail separation of 4.8 À. No other peaks are observed, due to the absence of long-range intercolumn ordering of the molecules.

All the reflections observed in the Dhd phase are also observed in the Dho phase. The

appearance of the (100) and (001) peaks above and below the phase transition is shown in the left and middle columns of figure 4. The integrated intensities do not change appreciably through the transition, although the (001) peak sharpens to become resolution limited in the

Dho phase. Figure 5 shows the intercolumnar distance d, calculated from the position of the triangular (100) peak, as a function of temperature. The dramatic negative thermal coefficient of expansion in the Dhd phase is most likely the consequence of the hydrocarbon tails becoming stiffer and therefore longer with decreasing temperature. Indeed, the same effect

may provide the driving mechanism for the Dhd --+ Dh. transition ; as tail conformational

degrees of freedom are « frozen out », steric hindrance between tails in adjacent columns

should become more important, resulting in enhanced column-column coupling. This hypothesis is strengthened by the observation that the diffuse hydrocarbon-tail diffraction at 1.3 A -1 is weaker in the Dho phase than in the Dhd phase. (The diffuse maximum in the

Dho phase is also essentially isotropic, rather than being centered off-axis ; it can be described

empirically by a functional form

Extrapolation of d vs. T from the Dhd phase to the constant value measured in the

Dho phase indicates that we may be close to a second-order transition. which is however

(10)

Fig. 4.

-

Scattering profiles at three temperatures upon heating through the coexistence region at the Dhd --+ Dho phase transition. The double-peaked (100) profiles indicate the progress of the transition

(left). The sharp (001) peak of the Dh. phase weakens upon heating (center panel, top), and is replaced

in the Dhd phase by a broadened diffuse peak (bottom center panel, note expanded qz axis). At right,

scans along the qy direction with fixed qx

=

0, qz = 1.727 Â- show the transverse evolution of the (001)

peak and the superlattice and peaks.

Fig. 5.

-

Intercolumn distance d, as derived from the fundamental (100) peak, versus temperature.

Closed circles indicate measurements made on warming, open circles measurements on cooling. Where

two solid circles are shown at the same temperature, two distinct peaks were visible in the diffraction pattern, as shown in figure 4, indicating coexistence. Solid line is the result of a least-squares fit to the

measured distances ; above 75 C it has a slope of - 0.037 À/C.

(11)

preempted by a first-order jump. However, a superlattice peak intensity (see below) would be

a better choice for an order parameter than d. All peak positions, including those of the new

peaks discussed below, are essentially temperature-independent in the Dho phase ; the length

of the fundamental (100) vector is q 1

=

0.334 Â-1.

Upon formation of the Dho phase, a number of new reflections appear, as indicated by the

open circles indicated in figure 3. All the reflections in the Dho phase are resolution-limited, indicating correlation lengths of at least 800 Â. We will continue to use the triangular (HKL ) Bragg indices of the Dhd phase to describe these reflections. New reflections in planes

at qz = 0.654 Â -1, 1.309 A-1 and 1.727 Â -1 correspond to L

=

0.379, L

=

0.758 and

L

=

1. The first two values are very close to L = 3/8 and L

=

6/8, but careful measurements of vector differences associated with reflection through the qz

=

0 plane have verified that the

peaks consistently deviate from these commensurate positions by at least one FWHM [11].

There is thus some type of incommensurate modulation along the columnar axis. No new

peaks are seen along the [0 0, L meridional axis. In the qx and qy directions, the new

reflections correspond to a 3 x 3 R 30° superlattice, i.e. the new fundamental is indexed

as a 1 1 0 33 3 ). The new unit cell therefore consists of three columns. The evolution of some of these superlattice peaks at the Dhd-Dho phase transition is shown in the right-hand column of figure 4. The absence of any new peaks in the equatorial (HKO ) plane implies that the

electron density projections of the three columns onto the basal plane are identical, and therefore that the superlattice ordering does not entail any distortion of the underlying hexagonal mesh.

The reflections in the L

=

0.379 and L

=

0.758 planes, and the absence of any peaks in

these planes along the (OOL ) axis, are consistent with an incommensurate helical arrangement of molecules within the columns. Indeed, helical order has previously been observed in columnar phases of discotic and cone-shaped molecules [14, 15]. In most of these

measurements the phase of the helix was uncorrelated from column to column, resulting in

diffuse layer lines, though in one case [15] additional Bragg peaks were also reported. Semi- empirical conformational analyses [16] of triphenylene derivatives similar to HHTT have indicated that adjacent molecules along a column minimize steric hindrance via a relative rotation of roughly 45°. Alternate tails around the circumference of each molecule tilt above and below the plane of the core, so that once the initial clockwise-counterclockwise symmetry is broken the helical order can extend to large distances. This analysis is supported by the

results for the HHTT molecule as obtained from the structure in the K phase (see Sect. 4).

The diffraction pattern for a group of atoms repeated along the z-axis by the operation of a non-integer screw is well-known [17] : diffraction maxima are found at

where m and n are integers, P is the pitch of the helix, and p is the rise per subunit. In the present case, the intracolumn molecular spacing is p

=

2 ’TT / (1.727 A-1 )

=

3.638 A, and the pitch is given by P

=

6 ’TT / (0.654 A -1)

=

28.82 A

=

7.92 p, corresponding to a 45.50 rotation

between adjacent molecules. This means that the minimum correlation length of 800 A

mentioned earlier comprises at least 220 molecules or about 30 complete rotations.

The superlattice order is associated with groups of three columns forming triangles. Within

a group of three columns, we can assign to the molecules in each individual column an overall vertical displacement and helical phase. Without going into the details of the model to be discussed in section 5, it is clear that the superlattice ordering must involve both the helical

phase differences and the vertical displacements, since superlattice peaks are seen in the

(n

=

0 ; m = 1) plane as well as in the (n

=

3, 6 ; m

=

0) planes.

(12)

4. Structure of the K phase.

The unit cell was determined to be monoclinic :

From the systematic absences HKL : H + K = 2 n + 1 and HOL : L

=

2 n + 1 the space group was either acentric Cc or centric C2/c. The structure was solved in the acentric space group Cc by the use of the MULTAN 11/82 program package which revealed the locations of 32 atoms. The remaining atoms were found from weighted Fourier syntheses. This structure

revealed the presence of a molecular 2-fold axis, so structure refinement was performed in the

centric space group C2/c by full-matrix least squares techniques. The hydrogen atoms were

included in pre-calculated positions but were not refined. The refinement converged to

R = 0.066 and RW = 0.077.

Half of the unit cell is shown in figure 6b. Note that there are 4 molecules per unit cell,

which are positioned in pairs on top of each other. These pairs are separated by c/2, and hence the molecules are regularly spaced in the direction along the c-axis. This situation is very different from that in the related hexa-alkyltriphenylenes where it has been found that two relatively close molecules are in turn rather widely spaced from the next pairs

in the direction perpendicular to the discs [18]. In the HHTT K phase the two molecules in a

pair are rotated by 180° with respect to each other, so that we can say that the columns have a

Fig. 6.

-

Structure of the K phase. (a) Stereoscopic view of an individual molecule. Ellipses indicate

r.m.s. amplitudes of anisotropic displacements ; (b) one half of a unit cell, viewed along the c axis.

Atoms in the upper plane are indicated with closed circles, atoms in the lower plane with open circles.

(13)

helical structure with a pitch P

=

2 c. The ratio a/b = 1.13 found for the unit cell is far away from triangular symmetry which requires alb

=

0. However, the fundamental spacing

between the molecular planes parallel to the diagonal of the unit cell can be calculated to be 18.8 Â, which exactly equals the spacing in the Dho phase. This explains the constancy through all three phases of the position of the low-angle diffraction peak reported for powder X-ray results [10]. Hence the K - Dho transition can be accomplished by a relatively small parallel displacement of molecules. In addition, of course, the angle {3 should then change

from its value of 97.85° in the K-phase to 90°.

A stereoscopic picture of the HHTT-molecule in the K-phase is shown in figure 6a. The

structure of the 18 core carbon atoms is quite close to that of the simple triphenylene molecule [19]. Note that there is only one 2-fold axis in the plane of the molecule. The two pairs of alkyl

chains close to this axis tilt out of the central molecular plane in opposite directions. The

remaining two alkyl chains do not show this behavior. Root-mean-square (r.m.s.) motional amplitudes range from roughly 0.25 Â for the core atoms to almost 1.0 Â for the carbon atoms near the ends of the alkyl tails ; evidently, there is considerable thermal motion of the

alkyl chains even in the K-phase.

The HHTT molecule has an intrinsic D3 h symmetry. However, examination of simple space-filling models shows that adjacent tails interfere with each other. Thus, alternate alkyl

tails are likely to tilt above and below of the plane of the triphenylene core, leading to a propellor-blade like molecule. This type of arrangement has also been found by semi- empirical conformational analyses of related triphenylene derivatives [16]. Alkyl chain tilting

will break the reflection symmetry of an isolated molecule, leading to D3 symmetry (one 3-

fold axis and three 2-fold axes). In the K phase, this symmetry is further broken due to the monoclinic environment, but at the K - Dho phase transition, the monoclinic environment of

a molecule is replaced by a triangular environment. We expect that the conformation of the HHTT molecule will then revert to D3 symmetry ; a propellor-blade like structure can then

lead to helical structure along the column.

5. Model of the Dho phase.

We now discuss the models used for least-squares analysis of diffraction data in the

Dho phase. The molecules lie on a lattice defined by real-space triangular vectors a and b and

columnar translation vector c. Following Cochran et al. [17], atoms are considered to lie along

sets of concentric helices, each of which is defined by the equations x

=

r cos (2 ’TT’Hz / P + cpo) and y=rsin(2’TT’Hz/P+CPo). H=:tl determines the sign of the helicity and CPo is an arbitrary helical phase. If a given set of atoms are spaced periodically along the

2-direction at positions Zk

=

Zo + k x p, then the structure factor is given by the convolution of the transform of the continuous helix and the transform of a set of planes with spacing p.

This gives

where m and n are integers, Jn is the n’th order Bessel function, and tan gi

=

qy/qx. As

discussed in section 3, the spacing is given by p = 3.638 Á, and the pitch is P =

28.82 À. We can model a single helical column of molecules by N coaxial discontinuous helices, where N is the number of atoms per molecule. If the position of the j’th atom in the

molecule is given in cylindrical coordinates by (pl, Oj, zj), with associated atomic form factor

fj (q), and we assume for generality a helical-phase preserving overall translation by

(14)

Zo 2, then the structure factor for a given (n ; m) reflection is given by

Note that Wo and Zo affect scattered phases, but not amplitudes. However, rotational and translational fluctuations will affect the experimental intensities differently. Also, if different columns have unequal heights or phases then interference can result in superlattice

diffraction.

The HHTT molecule (Fig. 7a) was assumed to retain its intrinsic D3 symmetry, as discussed

in the previous section. The molecule can then be decomposed into three pairs « t » of units,

t

=

0, 1, 2. The pairs are related by 2 ir/3 rotations, and we assume that the units are

symmetric within each pair : relative to the 2-fold rotation axis bisecting the pair

(0j, z) = (2 rt/3 ± 0,, ± Hzs), s = 1, 2, ..., M, and there are M

=

N/6 atoms in each unit.

(This implies an alternating propellor-blade tilt of the tails, as discussed above. We assume

that if the helicity of the column changes sign, then the helicity of the individual molecules

Fig. 7.

-

Structure of the Dho phase. (a) Best fit to molecular conformation, drawn to scale. Atoms are

numbered for reference in the text. 8cs is the angle between the sulphur atom Si and the first tail carbon atom ; Occ is the angle between adjacent carbons, assumed to be the same for all tail carbon atoms.

Adjacent tails are tilted by --t Ot above and below of the plane of the paper ; (b) proposed structure of

the 3-column superlattice (not to scale). Column 0 has the opposite helicity from columns 1 and 2, and is

displaced by p/2 from those columns.

(15)

also does.) Thus, the structure factor becomes

which factors into

The last term amounts to a selection rule : n must be a multiple of 3.

At this point the first problem encountered in the data analysis becomes apparent. The

structure factor is given by a sum of 10 or more Bessel functions, each of which is an

oscillatory function. In the traditional analysis of helical biological molecules such as proteins,

the subunit giving rise to the helical layer lines typically comprises a small fraction of the total molecule, and can be considered to lie at a well-defined radius. By contrast, in the present

case all atoms contribute more or less equally to the helical diffraction, and therefore all 10 Bessel functions, with different periodicities, contribute to the intensity (which is only

measured at Bragg peaks). This results in a large number of local minima in a least squares fit,

and considerable care is required to ensure that the final result is not only physically plausible

but also the best fit.

As seen in equation (7), the helical sign and phase of a single column cannot be determined from diffraction measurements, since these are reflected only in scattered phase differences.

However, if different columns have different phases and/or helicities, the interference of these can result in new superlattice peaks, and just such differences are implied by the

w5 x 13 superlattice peaks seen for n # 0. An additional possibility, as discussed in an

earlier paper [11], is that one or more columns might have random average helicity. The

Ô x J3 superlattice order in the Dho phase is associated with groups of three columns k

=

0, 1, 2. Within each group of three columns, we assign the molecules in column k an overall rotational-phase-preserving displacement Zk along the column, a displacement

Pk in the equatorial direction, and helical sign and phase Hk and ek : the equatorial displacement adds a factor exp (iqb - Pk) to the single-column structure factor phase in equation (7). The equatorial displacements are given by po

=

0, pl

=

a, p2

=

b. Without loss of generality, we can take 00

=

0 (or random), Ho = 1 and Zo

=

0. (Of course, because of the 3-fold symmetry of the molecules, rotations are only defined modulo 120°). We further

assume that the heights of columns 1 and 2 are symmetric with respect to column 0, i.e.

Zl - Z = - Z2.

Initial calculations were done with the Zk taken as adjustable variables. However, it was

found that the fitted values of the Zk were quite insensitive to details of the molecular

conformation. The nonzero intensity of the (001 ) peak rigorously excludes Z

=

p /3, while

(16)

the nonzero intensity of the 111 ( 33 peaks excludes Z = 0. Fits to the entire set of Bragg peak intensities consistently give 0.45 p , Z 10.55 p ; Z is probably exactly equal to p/2 and was fixed at this value in subsequent fits. This implies that columns 1 and 2 are at the

same height, and form a sublattice of molecules all at the same height. Column 0 forms part of

a second sublattice of molecules, all at height Zo

=

0. If we then fix Zl

= -

Z2

=

p /2, the terms involving Z reduce to factors of exp (i 2 7TmZ / p) = (- 1 )"’ in the appropriate

places. Combining the phase factors for the different columns, after a certain amount of manipulation (see Appendix) we arrive at the following expression for the unit cell structure factor :

where

The calculated intensity was obtained by squaring the total structure factor and multiplying

it by a normalization factor Io, a Lorentz-polarization factor H, and a Debye-Waller factor U.

Taking into account the partial polarization of the beam by the monochromator and analyser crystals, and the anisotropic resolution function, an appropriate Lorentz-polarization factor

was given by

with the angular widths determined by the mosaic and instrumental resolution, as discussed in section 2 :

Several different forms for the Debye-Waller factor were tested. While at first it might

seem logical to use a factor of the form exp (- (q u )2 ), where the qi and ui are Cartesian coordinates, this neglects the fact that a simple translation of an individual molecule along a

column breaks both translational and helical symmetry. A more natural choice is to use the

same cylindrical coordinates used for the structure calculation, and to use helical-phase- preserving translations Z. An appropriate Debye-Waller factor is then

u, clearly measures the extent of random motion in the equatorial plane, which we assume to

be isotropic. um measures the extent of phase-preserving vertical motion (we can think of the

atoms « sliding along a helical wire »). u,, measures the extent of purely rotational

(17)

fluctuations. Unm measures the extent to which the vertical and rotational motions are

coupled ; it can range from --t 2 1 u,, u,,, 1 (perfectly correlated or anticorrelated) to zero.

Putting everything together, the scattered intensity is given by :

where {GJ spans the V3 x V3 R 300 superlattice reciprocal lattice.

The quantitative analysis of the helical and superlattice ordering was quite sensitive to

estimates of the molecular conformations. However, the residual uncertainty in our integrated peak intensities and the lack of data beyond 2 Á - prevented a direct determination of detailed atomic coordinates in the Dho phase. In most cases we used bond distances derived from our crystallographic measurement of the K phase, averaged to reflect D3 symmetry. The following assumptions were made about the structure of the HHTT molecule in the

Dho phase (Fig. 7a) : 1) Molecules in all three columns were assumed to have identical

conformations, aside from possible reversals of helicity. 2) The inner core carbon and sulphur

atoms (Cl, C2, C3 and SI) were assumed to have bond lengths given by the K-phase data ; a typical carbon-carbon distance is 1.45 Á. (It should be noted that if this bond distance was

made a free parameter in the fits it typically converged to a somewhat smaller and unphysical

value of 1.1 À.) The sulphur atom was assumed to lie in the plane of the triphenylene core, as

in the K-phase structure. 3) The carbon atoms C4-C9 in each tail were considered to lie in a

plane which was tilted out of the triphenylene core plane by an angle ± et. The angle between

the sulphur-carbon bonds C3-Sl and S1 - C4 was taken to be a free parameter, Ocs. The

carbon atoms were assumed to have an all-trans configuration in the chain, as shown in figure 7. The carbon-carbon bond distances were all fixed ait 1.485 Â ; the angles between adjacent carbon bonds along the tail were assumed to all be equal to a free parameter,

Table II. - Parameters giving ’rise to the fit in table 1.

(18)

Occ. This is clearly â somewhat limited model for the alkyl tails ; for example, it does not

allow for the possibility of gauche conformations. However, the goal was to arrive at

reasonable agreement between theory and data with the smallest number of adjustable parameters. Occ thus effectively controlled the length of the alkyl tail. Typical fits to the data gave 0,

=

10° ± 5, Ocs

=

80° ± 10 and Occ

=

110° ± 20. Note that this value for ecc is exactly what one would expect _ on the basis of a normal all-trans configuration.

Also, in some fits we allowed the molecules to rotate a small amount randomly about

random axes in the a-b plane, similar to the tilting motion which, if correlated, would result in

a Drd phase [5]. Treated as a free parameter, this molecular tilt typically converged to a value

of about 3.5° ; it was not strongly correlated with other parameters. We did not consider models in which the molecular tilt was correlated with the column helicity.

The Debye-Waller terms typically converged to ur - 2 Â, um - 1.0 and un _ 0.15. The first two terms correspond to r.m.s. positional motion in both the basal and columnar directions of

1-2 Â : a fairly large amplitude motion compared with the 3.64 À molecular spacing along the

columns. The third term corresponds to r.m.s. rotational fluctuations on the order of 5-10°

about the z-axis. In this context it is interesting to note that apart from (n = 3, 6 ;

m

=

0) no other helical peaks were observed, even though scattering in the planes (n = - 6 ; m = 1), (n = - 3 ; m = 1) and (n = 9 ; m = 0) planes (L = 0.253, 0.623 and 1.139) are allowed by symmetry. The absence of observed peaks in the n

=

9 plane is simply explained by the rapid decay in amplitude of the Jn Bessel function with increasing n.

However, the n

= -

3 and n

= -

6 planes should have the same intrinsic intensities as their

n

=

3. and n

=

6 counterparts. The absence of observed peaks in these planes is best explained by correlated fluctuations, i. e. a negative value for Unm. This most likely results from

fluctuations in which the molecules, rather than moving vertically along the helical trajectory (un

=

0) or have a pure vertical motion, rotate opposite to the helical trajectory while moving vertically. This type of motion allows the tails of fluctuating molecules to move into the gaps between the tails of the molecules above or below them.

The formation of the three column unit cell in the Dho structure can be understood on the basis of steric frustration of the molecular tails. The intercolumn separation in the Dho phase is 5-15 % smaller than the diameter of the HHTT molecule with the tails fully

extended. This implies that either the molecules must be at. different heights, forming an overlapping structure, or that if the molecules are at the same height, the tails must interlock

in a gear-like fashion. Molecular interdigitation in a triangular lattice is frustrated in the sense

that it is not possible to have all the neighbors of a molecule translated by ± p /2. (This

situation is in fact isomorphous to the antiferromagnetic Ising model on a triangular lattice ;

structures quite similar to the one described below have been observed [20] in linear-chain magnets where the chains make a hexagonal lattice and there is antiferromagnetic coupling in

the basal plane.) Further frustration is introduced by the rotational degrees of freedom : while it is possible to construct an interlocking triangular mesh Qf gears, they cannot then rotate.

This frustration is partially relieved by the formation of two sublattices at different heights.

Once these sublattices have formed, it is clear that the behavior of molecules in column 0 may be quite different from that of molecules in the other two columns, and that these differences may result in a superlattice ordering of the helical phases.

The superlattice ordering reflected in the n =1= 0 planes must result from some difference in helical signs or phases of the different columns. To account for all degrees of freedom in the unit cell, we must include for each of the three columns a helical sign Hk, helical phase CPk’ and vertical displacement Zk. As previously discussed, we set Ho

=

1, eo

=

0,

Zo

=

0 and Z1 = - Z2 = p/2, thus the remaining models have definite Hl, H2, 403A61 and

03A62. Additionally , it is possible that one or more columns rotate freely or have random

Références

Documents relatifs

Namely, we show that for any given Lasso regularization parameter λ and any observed data y belonging to a set of full (Lebesgue) measure, the cardinality of the support of a

In addition to the parameters usually considered, like the geometry of the mean flow [4, 5] or the magnetic boundary conditions [6, 7], the turbulent fluctuations of the flow seem

We show that under a suitable condition on the design matrix, the number of nonzero coefficients of the Lasso solution is an unbiased estimate for the degrees of freedom.. An

Vaiter S, Deledalle C, Peyr´ e G, Fadili J, Dossal C (2012b) Local behavior of sparse analysis regularization: Applications to

In the special case of standard Lasso with a linearly independent design, (Zou et al., 2007) show that the number of nonzero coefficients is an unbiased esti- mate for the degrees

To investigate the effect of the loss of this degree of freedom, we have considered a simple case of a melt of polymer chains where one end of each chain is anchored to a fixed point

depends on the signs of the Burgers’ vector and of the strain. For small strains the process necessitates some acti- vation energy; there is a critical strain above

depends on the signs of the Burgers’ vector and of the strain. For small strains the process necessitates some acti- vation energy; there is a critical strain above