arXiv:2608.20449·v1·cond-mat.soft
The friction-era VOS amplitude of a string network from nematic disclination data
Dimitrios Efstratiou · Evangelos Achilleas Paraskevas · Leandros Perivolaropoulos
Abstract
A tangle of line defects coarsens as the mean spacing between neighbouring lines grows. In a viscous medium the motion is overdamped, and the velocity-dependent one-scale (VOS) model predicts a late-time attractor , with the ratio of line tension to drag and a dimensionless amplitude. The growth law holds for every value of the three model parameters---the momentum parameter , the sink coefficient , and the curvature ratio ---since all three enter only through , . Thus, the exponent constrains none of them, and the amplitude is the only quantity a density history can deliver. We measure it from the disclination data of Chuang, Turok and Yurke on a nematic liquid crystal, whose companion measurement of loop collapse fixes on the same samples, canceling the 5CB material constants. Treating the unmatched per-quench as a nuisance parameter with a Gaussian prior and marginalizing it analytically, we obtain from the three quenches in the m cell; the fourth, the only one in the thinner m cell, gives and is fitted separately. Converting either into requires , which these data do not determine, so the result is a curve, , not a number. At with they give and , against -- from relativistic simulations, values reached only at -- and --. We know of no VOS calibration for a cosmological network, so we cannot attribute the excess to topology, and we list what a repeat experiment must measure.
Comments: 16 pages, 6 figures, the numerical analysis files for the production of the figures can be found in the following github repository: https://github.com/Dimitrios1993/friction-era-vos-amplitude-z2-nlc