English

Phase equilibration in bubble collisions

High Energy Physics - Phenomenology 2011-08-01 v1 Astrophysics

Abstract

In the context of an Abelian gauge symmetry, spontaneously broken at a first-order transition, we discuss the evolution of the phase difference between the Higgs fields in colliding bubbles. We show that the effect of dissipation, represented by a finite plasma conductivity, is to cause the phases to equlibrate on a time-scale, determined by the conductivity, which can be much smaller than the bubble radii at the time of collision. Currents induced during the phase equilibration generate a magnetic flux, which is determined by the initial phase difference. In a three-bubble collision, the fluxes produced by each pair of bubbles combine, and a vortex can be formed. We find that, under most conditions, the probability of trapping magnetic flux to form a vortex is correctly given by the ``geodesic rule''.

Keywords

Cite

@article{arxiv.hep-ph/9501266,
  title  = {Phase equilibration in bubble collisions},
  author = {T. W. B. Kibble and Alexander Vilenkin},
  journal= {arXiv preprint arXiv:hep-ph/9501266},
  year   = {2011}
}

Comments

20 pages, REVTEX