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Scaling of cosmological domain wall networks with junctions

2006/12/15 by P. P. Avelino, C. J. A. P. Martins, J. Menezes +2 · 4 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1016/j.physletb.2007.02.025

published as Phys.Lett.B647:63-66,2007 · 4 pages, 2 figures

arxiv created 2006/12/15 · openalex publication_date 2007/02/17 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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 N of coupled scalar fields, approaches the so-called `ideal' model (in terms of its potential to lead to network frustration). We consider values of N 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 N. These results strongly support our no-frustration conjecture.

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