Evolution of current-carrying string networks

• Type: Another Publication in an International Scientific Journal
• Date: 2024-06-10

Authors

José Ricardo Correia (Author) Other; Martins, CJAP (Author) FCUP; Francisco Pimenta (Author) FEUP

Journal

Title: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

Vol. 855

Pages: 1-7

ISSN: 0370-2693

Publisher: Elsevier

Indexing

ISI Web of Knowledge - 0 Citations

Scopus - 0 Citations

Other information

Authenticus ID: P-010-KF6

DOI: 10.1016/j.physletb.2024.138788

Abstract (EN): 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 modelling.

Language: English

Type (Professor's evaluation): Scientific

No. of pages: 7