Scaling in necklaces of monopoles and semipoles
Mark Hindmarsh, Anna Kormu, Asier Lopez-Eiguren, David J. Weir

TL;DR
This paper uses large-scale simulations to show that cosmic necklaces with monopoles or semipoles maintain a constant density relative to the universe's background, confirming their scaling behavior and providing new insights into pole annihilation processes.
Contribution
It provides the first large-scale simulations of semipoles in cosmic necklaces, demonstrating their scaling behavior and proposing a diffusive process for pole annihilation.
Findings
Networks of cosmic necklaces approach scaling, maintaining constant energy density fractions.
Number of monopoles or semipoles per unit string length remains constant over time.
Simulation results do not match existing analytical models, suggesting new physics.
Abstract
Models of symmetry breaking in the early universe can produce networks of cosmic strings threading 't Hooft-Polyakov monopoles. In certain cases there is a larger global symmetry group and the monopoles split into so-called semipoles. These networks are all known as cosmic necklaces. We carry out large-scale field theory simulations of the simplest model containing these objects, confirming that the energy density of networks of cosmic necklaces approaches scaling, i.e. that it remains a constant fraction of the background energy density. The number of monopoles per unit comoving string length is constant, meaning that the density fraction of monopoles decreases with time. Where the necklaces carry semipoles rather than monopoles, we perform the first simulations large enough to demonstrate that they also maintain a constant number per unit comoving string length. We also compare our…
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