On the Evolution of Abelian-Higgs String Networks
J. N. Moore, E. P. S. Shellard, C. J. A. P. Martins
TL;DR
This study investigates the scale-invariant evolution of Abelian-Higgs string networks using large-scale field-theory simulations in flat and expanding backgrounds, extracting the true invariant string length and rms velocity to test the velocity-dependent one-scale (VOS) model. The authors develop a robust diagnostic toolkit, including a novel fat-string algorithm, and show that loop production, supplemented by limited massive radiation, provides a consistent description of network decay across backgrounds. Analyses of flat-space, radiation-era, matter-era, and global-string systems reveal quantitative fits with VOS parameters (notably the loop chopping efficiency ${\tilde c}$ and radiation coefficients $\Sigma$ and $L_d$) that reproduce the observed evolution of the correlation length and velocity, while highlighting the role of proto-loops in energy losses. The results support the standard cosmological picture where loop production and gravitational radiation (and, for global strings, Goldstone boson radiation) govern scaling, with important implications for predicting cosmic-ray and gravitational signatures and for informing extrapolations from simulations to cosmological scales.
Abstract
We study the evolution of Abelian-Higgs string networks in large-scale numerical simulations in both a static and expanding background. We measure the properties of the network by tracing the motion of the string cores, for the first time estimating the rms velocity of the strings and the invariant string length, that is, the true network energy density. These results are compared with a velocity-dependent one scale model for cosmic string network evolution. This incorporates the contributions of loop production, massive radiation and friction to the energy loss processes that are required for scaling evolution. We use this analysis as a basis for discussing the relative importance of these mechanisms for the evolution of the network. We find that the loop distribution statistics in the simulations are consistent with the long-time scaling of the network being dominated by loop production. Making justifiable extrapolations to cosmological scales, these results appear to be consistent with the standard picture of local string network evolution in which loop production and gravitational radiation are the dominant decay mechanisms.
