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arXiv:astro-ph/0612444·v1·Astrophysics

Scaling of cosmological domain wall networks with junctions

P.P. Avelino🇵🇹 · C.J.A.P. Martins🇵🇹 · J. Menezes🇵🇹 · R. Menezes🇧🇷 · J.C.R.E. Oliveira🇵🇹

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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.

Comments: 4 pages, 2 figures

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