Bogomol'nyi equations for Dirac-Born-Infeld cosmic string
Handhika Satrio Ramadhan, M Naufal Athaullah, Ilham Prasetyo
TL;DR
This paper demonstrates that Dirac–Born–Infeld cosmic strings can possess Bogomol'nyi–Prasad–Sommerfield configurations if the scalar potential is chosen self-consistently. Using both the BPS Lagrangian method and a stressless energy–momentum approach, it derives exact first-order BPS equations and a trigonometric potential, with a tension that scales linearly with the winding number and deforms with the DBI parameter α. In the α → 0 limit, the results recover the Nielsen–Olesen vortex, confirming consistency with the Abelian–Higgs framework. The study reveals a sine-Gordon–like structure underlying the BPS DBI string and identifies regularity bounds that constrain α relative to β, providing a nuanced extension of BPS theory to nonlinear DBI dynamics.
Abstract
We revisit the question of whether Dirac-Born-Infeld (DBI) cosmic strings can admit Bogomol'nyi-Prasad-Sommerfield (BPS) configurations. Earlier work by Babichev et al. arXiv:0809.2013 concluded that DBI strings with the standard Mexican-hat potential possess no BPS limit, implying an unavoidable nonzero binding energy. In contrast, using the BPS Lagrangian method, we show that DBI strings do admit BPS solutions, provided the potential is chosen self-consistently. Imposing the existence of Bogomol'nyi equations uniquely determines the admissible potential and yields exact first-order BPS equations for DBI vortices. We independently verify the consistency of these equations using the stressless (vanishing-pressure) condition on the energy-momentum tensor. The resulting solutions saturate the Bogomol'nyi bound, exhibit zero binding energy, and smoothly recover the Nielsen-Olesen string in the limit $α\to 0$. Regularity of the gauge-field equation requires $α< π^2$. A notable outcome of the construction is that the BPS-compatible potential takes a trigonometric form closely related to the sine-Gordon potential, revealing a natural correspondence between the sine-Gordon string and the BPS DBI string. The BPS tension scales linearly with the winding number $n$ but acquires an $α$-dependent deformation.
