Dirac Born Infeld (DBI) Cosmic Strings
Eugeny Babichev, Philippe Brax, Chiara Caprini, Jerome Martin and, Daniele Steer

TL;DR
This paper explores the properties of cosmic strings within a Dirac-Born-Infeld (DBI) extension of the Abelian-Higgs model, revealing narrower cores, lower action, and non-BPS nature, with implications for string network behavior.
Contribution
It introduces a continuous DBI deformation of the Abelian-Higgs model, analyzes cosmic string solutions numerically, and discusses their stability and network dynamics.
Findings
DBI cosmic strings have narrower cores than Abelian-Higgs strings.
The action for DBI strings is smaller, suggesting easier formation.
DBI strings are non-BPS and do not form junctions when meeting.
Abstract
Motivated by brane physics, we consider the non-linear Dirac-Born-Infeld (DBI) extension of the Abelian-Higgs model and study the corresponding cosmic string configurations. The model is defined by a potential term, assumed to be of the mexican hat form, and a DBI action for the kinetic terms. We show that it is a continuous deformation of the Abelian-Higgs model, with a single deformation parameter depending on a dimensionless combination of the scalar coupling constant, the vacuum expectation value of the scalar field at infinity, and the brane tension. By means of numerical calculations, we investigate the profiles of the corresponding DBI-cosmic strings and prove that they have a core which is narrower than that of Abelian-Higgs strings. We also show that the corresponding action is smaller than in the standard case suggesting that their formation could be favoured in brane models.…
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