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Stretching and Kibble scaling regimes for Hubble damped defect networks

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Figure

Figure 1 depicts these diagnostics for all the expansion
Table I. Scaling properties of numerical simulations for domain wall networks with different expansion rates λ in the linearscaling regime
Figure 2.Results from velocity measurements for differentchoices of thresholds, illustrated in the top panel
Table II. The best-fit values for the free parameters of the extended VOS model in our present analysis; for comparison, wealso show the values obtained in our previous work [21]
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