Geometric theory of topological defects: methodological developments and new trends
arXiv:2301.01050 · doi:10.1080/21680396.2022.2163515
Abstract
Liquid crystals generally support orientational singularities of the director field known as topological defects. These latter modifiy transport properties in their vicinity as if the geometry was non-Euclidean. We present a state of the art of the differential geometry of nematic liquid crystals, with a special emphasis on linear defects. We then discuss unexpected but deep connections with cosmology and high-energy-physics, and conclude with a review on defect engineering for transport phenomena.
References in corpus (19)
- Traversable wormholes: Some simple examples
- General Relativity in Electrical Engineering
- Disclinations, dislocations and continuous defects: a reappraisal
- Pancharatnam-Berry phase optical elements for wavefront shaping in the visible domain: switchable helical modes generation
- The next generation of analogue gravity experiments
- On the deflection of light by topological defects in nematic liquid crystals
- Generation of vector beams with liquid crystal disclination lines
- Controllable shifting, steering, and expanding of light beam based on multi-layer liquid-crystal cells
- A locally finite model for gravity
- Cosmology in the laboratory: an analogy between hyperbolic metamaterials and the Milne universe
- Generation of hard twisted photons by charged particles in cholesteric liquid crystals
- Principles of thermal design with nematic liquid crystals
- Retrieving the saddle-splay elastic constant of nematic liquid crystals from an algebraic approach
- Thermal diode made by nematic liquid crystal
- Generation of optical vorticity from topological defects
- Probing the cosmological singularity with a particle
- Quantum influence of topological defects on a relativistic scalar particle with Cornell-type potential in cosmic string space-time with a spacelike dislocation
- The wiggly cosmic string as a waveguide for massless and massive fields
- Classical Kalb-Ramond field theory in curved spacetimes