Astrophysics > Cosmology and Nongalactic Astrophysics
[Submitted on 6 Aug 2021 (v1), last revised 14 Oct 2021 (this version, v2)]
Title:Charge-velocity-dependent one-scale linear model
View PDFAbstract:We apply a recently developed formalism to study the evolution of a current-carrying string network under the simple but generic assumption of a linear equation of state. We demonstrate that the existence of a scaling solution with non-trivial current depends on the expansion rate of the universe, the initial root mean square current on the string, and the available energy loss mechanisms. We find that the fast expansion rate after radiation-matter equality will tend to rapidly dilute any pre-existing current and the network will evolve towards the standard Nambu-Goto scaling solution (provided there are no external current-generating mechanisms). During the radiation era, current growth is possible provided the initial conditions for the network generate a relatively large current and/or there is significant early string damping. The network can then achieve scaling with a stable non-trivial current, assuming large currents will be regulated by some leakage mechanism. The potential existence of current-carrying string networks in the radiation era, unlike the standard Nambu-Goto networks expected in the matter era, could have interesting phenomenological consequences.
Submission history
From: Ivan Rybak [view email][v1] Fri, 6 Aug 2021 14:42:35 UTC (1,800 KB)
[v2] Thu, 14 Oct 2021 15:39:08 UTC (1,801 KB)
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