Abelian Higgs Cosmic Strings: Small Scale Structure and Loops
Mark Hindmarsh, Stephanie Stuckey, and Neil Bevis

TL;DR
This study uses lattice simulations of the Abelian Higgs model to analyze small scale structures and loop distributions in cosmic string networks, confirming some analytic predictions and revealing differences from Nambu-Goto models.
Contribution
It provides the first detailed field theory simulation of small scale structure and loop distributions, challenging existing analytic models and Nambu-Goto simulations.
Findings
Confirmed power-law two-point correlation function consistent with analytic predictions.
Found a very low loop number density of about 1 per horizon volume, contrasting Nambu-Goto results.
Identified a strong energy loss mechanism not involving width loops, supporting a scaling network without gravitational radiation.
Abstract
Classical lattice simulations of the Abelian Higgs model are used to investigate small scale structure and loop distributions in cosmic string networks. Use of the field theory ensures that the small-scale physics is captured correctly. The results confirm analytic predictions of Polchinski & Rocha [1] for the two-point correlation function of the string tangent vector, with a power law from length scales of order the string core width up to horizon scale with evidence to suggest that the small scale structure builds up from small scales. An analysis of the size distribution of string loops gives a very low number density, of order 1 per horizon volume, in contrast with Nambu-Goto simulations. Further, our loop distribution function does not support the detailed analytic predictions for loop production derived by Dubath et al. [2]. Better agreement to our data is found with a model…
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