Sh. Lee et al., MOLECULAR-DYNAMICS AND ORDERING OF SIDE-CHAIN LIQUID-CRYSTAL POLYMERSAS STUDIED BY PARAMAGNETIC-RESONANCE, Liquid crystals, 18(3), 1995, pp. 495-502
Molecular dynamics of side chain liquid crystalline polymers (LCP) and
their components were studied using the technique of paramagnetic res
onance. A cigar shape spin probe (COL) and a nearly spherical spin pro
be (TPL) were used to study the motions and order of the LCPs. Compute
r simulations of the observed spectra were performed. Both rotational
correlation times and order parameters were extracted from these simul
ations. We found that LCPs containing 30 per cent and 50 per cent of m
esogenic side chains had about the same viscosity as indicated by near
ly equal tumbling times at the same temperature. In addition, the LCPs
motion is considerably slower than that of the monomeric liquid cryst
al indicating that the spacer couples the motions of the side chains t
o those of the main chain. Rotations about axes perpendicular to the s
ide chain are slowed more than rotations about an axis parallel to the
side chain. DSC measurements were employed to study the phase transit
ions. The 30 and 50 per cent LCPs displayed first order NS, transition
s, but the 50 per cent LCPs transition was much weaker, in agreement w
ith McMillan's theory which predicts a first order transition for T-NS
/T-NI>0.87 (observed ratios are 0.98, 0.90 and 0.86 for 30, 50 and 100
per cent LCPs, respectively). The 30 per cent LCP has a very short ne
matic range so that the nematic order, which is not saturated at the N
S transition, can couple with the smectic order. This was indicated by
a sharp change in slope of the order parameter versus temperature plo
t as the smectic is entered. The LCPs studied formed a highly ordered
glass when cooled in a 1 T field. If one could find a LCP with similar
ordering properties whose glass temperature is well above room temper
ature, then one would have a useful binder for the manufacture of haze
-free polymer dispersed liquid crystal displays.