Abstract (EN):
We study a number of domain wall forming models where various types of defect junctions can
exist. These illustrate some of the mechanisms that will determine the evolution of defect networks
with junctions. Understanding these mechanisms is vital for a proper assessment of a number
of cosmological scenarios: we will focus on the issue of whether or not cosmological frustrated
domain wall networks can exist at all, but our results are also relevant for the dynamics of cosmic
(super)strings, where junctions are expected to be ubiquitous. We also define and discuss the
properties that would make up the ideal model in terms of hypothetical frustrated wall networks, and
provide an explicit construction for such a model. We carry out a number of numerical simulations
of the evolution of these networks, analyze and contrast their results, and discuss their implications
for our no-frustration conjecture.
Language:
Portuguese
Type (Professor's evaluation):
Scientific