Evolution of Cosmic Necklaces and Lattices
arXiv:1009.1707 · doi:10.1103/PhysRevD.82.067301
Abstract
Previously developed analytic models for the evolution of cosmic string and monopole networks are applied to networks of monopoles attached to two or more strings; the former case is usually known as cosmic necklaces. These networks are a common consequence of models with extra dimensions such as brane inflation. Our quantitative analysis agrees with (and extends) previous simpler estimates, but we will also highlight some differences. A linear scaling solution is usually the attractor solution for both the radiation and matter-dominated epochs, but other scaling laws can also exist, depending on the universe's expansion rate and the network's energy loss mechanisms.
4 pages
References in corpus (5)
Cited by in corpus (8)
- Beyond the Standard Models with Cosmic Strings
- Monopoles on strings
- Numerical simulations of necklaces in SU(2) gauge-Higgs field theory
- Instability of Higgs Vacuum via String Cloud
- Scaling in necklaces of monopoles and semipoles
- Can Superconducting Cosmic Strings Piercing Seed Black Holes Generate Supermassive Black Holes in the Early Universe?
- Evolution of FLRW spacetime after the birth of a cosmic string
- Scaling properties of cosmic (super)string networks