Measuring Global Monopole Velocities, one by one

TL;DR

This paper introduces a new method for estimating individual global monopole velocities in a network, resolving previous uncertainties and providing insights into their scaling behavior in cosmology.

Contribution

The authors develop a novel technique to measure monopole velocities individually, improving accuracy and enabling detailed microphysics analysis in large-scale simulations.

Findings

No evidence of luminal monopole velocity branch.

Estimated parameters for the velocity-dependent one-scale model.

Validated the new method against existing estimators.

Abstract

We present an estimation of the average velocity of a network of global monopoles in a cosmological setting using large numerical simulations. In order to obtain the value of the velocity, we improve some already known methods, and present a new one. This new method estimates individual global monopole velocities in a network, by means of detecting each monopole position in the lattice and following the path described by each one of them. Using our new estimate we can settle an open question previously posed in the literature: velocity-dependent one-scale (VOS) models for global monopoles predict two branches of scaling solutions, one with monopoles moving at subluminal speeds and one with monopoles moving at luminal speeds. Previous attempts to estimate monopole velocities had large uncertainties and were not able to settle that question. Our simulations find no evidence of a luminal branch. We also estimate the values of the parameters of the VOS model. With our new method we can also study the microphysics of the complicated dynamics of individual monopoles. Finally we use our large simulation volume to compare the results from the different estimator methods, as well as to asses the validity of the numerical approximations made.