Current-carrying string network evolution in an external magnetic field
P. B. Barbosa, C. J. A. P. Martins

TL;DR
This paper extends the Charge-Velocity dependent One-Scale (CVOS) model for superconducting cosmic strings by including interactions with an external magnetic field, analyzing how this affects the network's evolution and energy dynamics.
Contribution
It introduces a phenomenological extension to the CVOS model to incorporate external magnetic field interactions, revealing new possible energy gain mechanisms for the string network.
Findings
Identification of a new scaling solution where the network gains energy from magnetic field interactions.
Classification of physically allowed scaling solutions under the extended model.
Analysis of the magnetic field's impact on charge and current evolution in the network.
Abstract
Cosmic strings are topological defects arising in a variety of cosmological scenarios, as the Universe undergoes symmetry-breaking phase transitions, whose discovery would offer valuable insight into the high-energy physics that shaped the early Universe. To interpret such a detection, robust theoretical models are essential. The Velocity-dependent One-Scale (VOS) model is particularly prominent: it self-consistently treats the network as a thermodynamic system, characterizing its key properties, and predicting its large-scale evolution. This has recently been extended to include superconducting cosmic strings, which carry additional degrees of freedom, giving rise to the Charge-Velocity dependent One-Scale (CVOS) model. One limitation of the latter model is that it only included loss mechanisms for the charge and current. Here, we extend this model by phenomenologically including a…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Black Holes and Theoretical Physics
