  Cosmic string networks are expected to form in early Universe phase
transitions via the Kibble mechanism and are unavoidable in several Beyond the
Standard Model theories. While most predictions of observational signals of
string networks assume featureless Abelian-Higgs or Nambu-Goto string networks,
in many such extensions the networks can carry additional degrees of freedom,
including charges and currents; these are often generically known as
superconducting strings. All such degrees of freedom can impact the evolution
of the networks and therefore their observational signatures. We report on the
results of $2048^3$ field theory simulations of the evolution of a
current-carrying network of strings, highlighting the different scaling
behaviours of the network in the radiation and matter eras. We also report the
first numerical measurements of the coherence length scales for the charge and
current and of the condensate equation of state, and show that the latter
mainly depends on the expansion rate, with chirality occurring for the matter
era. Qualitatively, the fact that the matter era is the optimal expansion rate
for these networks to reach scaling is in agreement with recent analytic
modeling.
