Numerical simulations of necklaces in SU(2) gauge-Higgs field theory
arXiv:1611.08456 · doi:10.1103/PhysRevD.95.063520
Abstract
We perform the first numerical simulations of necklaces in a non-Abelian gauge theory. Necklaces are composite classical solutions which can be interpreted as monopoles trapped on strings, rather generic structures in a Grand Unified Theory. We generate necklaces from random initial conditions, modelling a phase transition in the early Universe, and study the evolution. For all cases, we find that the necklace system shows scaling behaviour similar to that of a network of ordinary cosmic strings. Furthermore, our simulations indicate that comoving distance between the monopoles or semipoles along the string asymptotes to a constant value at late times. This means that while the monopole-to-string energy density ratio decreases as the inverse of the scale factor, a horizon-size length of string has a large number of monopoles, significantly affecting the dynamics of string loops. We argue that gravitational wave bounds from millisecond pulsar timing on the string tension in the Nambu-Goto scenario are greatly relaxed.
15 pages, 8 figures; v2: Figs. 2 (bottom) and 4 (top) corrected, some discussion added, results unchanged, accepted by PRD
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- Gauge Kinetic Mixing and Dark Topological Defects
- Detection of Low Tension Cosmic Superstrings
- Abelian-Higgs Cosmic String Evolution with CUDA
- General purpose graphics-processing-unit implementation of cosmological domain wall network evolution
- Scaling in necklaces of monopoles and semipoles
- Evolution of Semilocal String Networks: II. Velocity estimators
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