Scaling of cosmological domain wall networks with junctions
arXiv:astro-ph/0612444 · doi:10.1016/j.physletb.2007.02.025
Abstract
We describe the results of the largest and most accurate three-dimensional field theory simulations of domain wall networks with junctions. We consider a previously introduced class of models which, in the limit of large number of coupled scalar fields, approaches the so-called `ideal' model (in terms of its potential to lead to network frustration). We consider values of between N=2 and N=20. In all cases we find compelling evidence for a gradual approach to scaling, with the quantitative scaling parameters having only a mild dependence on . These results strongly support our no-frustration conjecture.
4 pages, 2 figures
References in corpus (8)
- Is the Dark Matter a Solid?
- One-scale Model for Domain Wall Network Evolution
- The Cosmological Evolution of Domain Wall Networks
- Frustrated Expectations: Defect Networks and Dark Energy
- Understanding Domain Wall Network Evolution
- Defect Junctions and Domain Wall Dynamics
- Rigidity and stability of cold dark solid universe model
- Scaling Dynamics of Domain Walls in the Cubic Anisotropy Model
Cited by in corpus (26)
- Dynamics of domain wall networks with junctions
- The cosmological evolution of p-brane networks
- The effect of kinematic constraints on multi-tension string network evolution
- Rigorous theoretical constraint on constant negative EoS parameter and its effect for the late Universe
- Semiclassical decay of topological defects
- Domain wall network evolution in (N+1)-dimensional FRW universes
- Scalar and vector perturbations in a universe with discrete and continuous matter sources
- Dynamics of Biased Domain Walls and the Devaluation Mechanism
- Bifurcation and pattern changing with two real scalar fields
- Evolution of domain wall networks: the PRS algorithm
- Constructing networks of defects with scalar fields
- Impact of string and monopole-type junctions on domain wall dynamics: implications for dark energy
- Construction of topological defect networks with complex scalar fields
- Perfect fluids with as sources of scalar cosmological perturbations
- Formation and evolution of kinky vortons
- Charge, junctions and the scaling dynamics of domain wall networks
- Stability of winding cosmic wall lattices with X type junctions
- Simulating the symmetron: domain walls and symmetry-restoring impurities
- Exact solutions of domain wall junctions in arbitrary dimensions
- Dark matter from cosmic defects on galactic scales?
- The role of domain wall junctions in Carter's pentahedral model
- p-brane dynamics in N+1-dimensional FRW universes
- X-type and Y-type junction stability in domain wall networks
- Non-Relativistic Strings in Expanding Spacetime
- Cosmological Consequences of Topological Defects: Dark Energy and Varying Fundamental Constants
- Scaling properties of cosmic (super)string networks