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Gaugek-vortices

2007/11/11 by Eugeny Babichev, E. Babichev
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #astro-ph #hep-ph #hep-th

paper · pdf · doi:10.1103/physrevd.77.065021

published as Phys.Rev.D77:065021,2008 · 8 pages, 2 figures

arxiv created 2007/11/11 · openalex publication_date 2008/03/24 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We consider gauge vortices in symmetry-breaking models with a noncanonical kinetic term. This work extends our previous study on global topological k-defects [Phys. Rev. D 74, 085004 (2006), including a gauge field. The model consists of a scalar field with a noncanonical kinetic term, while for the gauge field the standard form of its kinetic term is preserved. Topological defects arising in such models, k-vortices, may have quite different properties as compared to standard vortices. This happens because an additional dimensional parameter enters the Lagrangian for the considered model---a kinetic mass. We briefly discuss possible consequences for cosmology, in particular, the formation of cosmic strings during phase transitions in the early universe and their properties.

Citations