Scaling of cosmological domain wall networks with junctions

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dc.creatorAvelino, P. P.
dc.creatorMartins, C. J. A. P.
dc.creatorMenezes, J.
dc.creatorMenezes, R.
dc.creatorOliveira, J. C. R. E.
dc.date2006-12-15
dc.date.accessioned2026-07-07T11:00:29Z
dc.date.available2026-07-07T11:00:29Z
dc.descriptionWe 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.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0612444
dc.identifierhttp://arxiv.org/abs/astro-ph/0612444
dc.identifierPhys.Lett.B647:63-66,2007
dc.identifierdoi:10.1016/j.physletb.2007.02.025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187687
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleScaling of cosmological domain wall networks with junctions
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