Compact-like vortices in isotropic curved spacetime

Abstract

We introduced a generalized Maxwell-Higgs model in a $(3+1)$ isotropic spacetime, and we found their stationary solutions using the BPS approach in curved spacetime. In order to investigate the compact-like vortices, we assume a particular choice for the generalization term. The model is controlled by a potential driven by a single real parameter that can be used to change the vortex solutions profile as they approach their bound values. Resembling some flat spacetime vortex solutions, our model tends to compress the vortices when the parameter $l$ increases. Through numerical analysis, we also show the energy behavior and the magnetic field of the model.

17 pages, 5 figures. To appear in Annals of Physics

References in corpus (4)

• From Kinks to Compactons
• Compact Chern-Simons vortices
• Topological first-order vortices in a gauged CP(2) model
• Charged Nielsen-Olesen vortices from a Generalized Abelian Chern-Simons-Higgs Theory

Cited by in corpus (3)

• Phase transitions in the logarithmic Maxwell O(3)-sigma model
• Geometrically contracted structure in teleparallel $f(T)$ gravity
• Exponentially generalized vortex