Temperature-dependent orientational ordering on a spherical surface modeled with a lattice spin model

Full text not archived in this repository.

Please see our End User Agreement.

It is advisable to refer to the publisher's version if you intend to cite from this work. See Guidance on citing.

Add to AnyAdd to TwitterAdd to FacebookAdd to LinkedinAdd to PinterestAdd to Email

Luo, A. M., Wenk, S. and Ilg, P. orcid id iconORCID: https://orcid.org/0000-0002-7518-5543 (2014) Temperature-dependent orientational ordering on a spherical surface modeled with a lattice spin model. Physical Review E. 022502. ISSN 1539-3755 doi: 10.1103/PhysRevE.90.022502

Abstract/Summary

We study the orientational ordering on the surface of a sphere using Monte Carlo and Brownian dynamics simulations of rods interacting with an anisotropic potential. We restrict the orientations to the local tangent plane of the spherical surface and fix the position of each rod to be at a discrete point on the spherical surface. On the surface of a sphere, orientational ordering cannot be perfectly nematic due to the inevitable presence of defects. We find that the ground state of four +1/2 point defects is stable across a broad range of temperatures. We investigate the transition from disordered to ordered phase by decreasing the temperature and find a very smooth transition. We use fluctuations of the local directors to estimate the Frank elastic constant on the surface of a sphere and compare it to the planar case. We observe subdiffusive behavior in the mean square displacement of the defect cores and estimate their diffusion constants.

Altmetric Badge

Item Type Article
URI https://reading-clone.eprints-hosting.org/id/eprint/37432
Identification Number/DOI 10.1103/PhysRevE.90.022502
Refereed Yes
Divisions Science > School of Mathematical, Physical and Computational Sciences > Department of Mathematics and Statistics
Publisher American Physical Society
Download/View statistics View download statistics for this item

University Staff: Request a correction | Centaur Editors: Update this record

Search Google Scholar