Abstract
We conduct an in-depth analysis of the electroclinic effect in chiral, ferroelectric liquid crystal systems that have a first-order smectic-–smectic- (Sm-–Sm-) transition, and show that such systems can be either type I or type II. In temperature-field parameter space type-I systems exhibit a macroscopically achiral (in which the Sm- helical superstructure is expelled) low-tilt (LT) Sm-–high-tilt (HT) Sm- critical point, which terminates a LT Sm-–HT Sm- first-order boundary. Notationally, Sm- or Sm- denotes the Sm- phase with or without a modulated superstructure. This boundary extends to an achiral-chiral triple point at which the macroscopically achiral LT Sm- and HT Sm- phases coexist along with the chiral Sm- phase. In type-II systems the critical point, triple point, and first-order boundary are replaced by a Sm- region, sandwiched between LT and HT Sm- phases, at low and high fields, respectively. Correspondingly, as the field is ramped up, the type-II system will display a reentrant Sm-–Sm-–Sm- phase sequence. Moreover, discontinuity in the tilt of the optical axis at each of the two phase transitions means the type-II system is tristable, in contrast to the bistable nature of the LT Sm-–HT Sm- transition in type-I systems. Whether the system is type I or type II is determined by the ratio of two length scales, one of which is the zero-field Sm- helical pitch. The other length scale depends on the size of the discontinuity (and thus the latent heat) at the zero-field first-order Sm-–Sm- transition. We note that this type-I vs type-II behavior in this ferroelectric smectic is the Ising universality class analog of type-I vs type-II behavior in XY universality class systems. Lastly, we make a complete mapping of the phase boundaries in all regions of temperature–field–enantiomeric-excess parameter space (not just near the critical point) and show that various interesting features are possible, including a multicritical point, tricritical points, and a doubly reentrant Sm-–Sm-–Sm-–Sm- phase sequence.
1 More- Received 19 January 2019
DOI:https://doi.org/10.1103/PhysRevE.100.022707
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