Deprecated: $wgMWOAuthSharedUserIDs=false is deprecated, set $wgMWOAuthSharedUserIDs=true, $wgMWOAuthSharedUserSource='local' instead [Called from MediaWiki\HookContainer\HookContainer::run in /var/www/html/w/includes/HookContainer/HookContainer.php at line 135] in /var/www/html/w/includes/Debug/MWDebug.php on line 372
Instability of electroweak homogeneous vacua in strong magnetic fields - MaRDI portal

Instability of electroweak homogeneous vacua in strong magnetic fields

From MaRDI portal
Publication:6508130

arXiv2211.00769MaRDI QIDQ6508130

I. M. Sigal, Adam Gardner


Abstract: We consider the classical vacua of the Weinberg-Salam (WS) model of electroweak forces. These are no-particle, static solutions to the WS equations minimizing the WS energy locally. We study the WS vacuum solutions exhibiting a non-vanishing average magnetic field of strength b, and prove that (i) there is a magnetic field threshold b* such that for b<b*, the vacua are translationally invariant (and the magnetic field is constant), while for b>b* they are not, (ii) for b>b*, there are non-translationally invariant solutions with lower energy per unit volume and with the discrete translational symmetry of a 2D lattice in the plan transversal to b, and (iii) the lattice minimizing the energy per unit volume approaches the hexagonal one as the magnetic field strength approaches the threshold b*. In the absence of particles, the Weinberg-Salam model reduces to the Yang-Mills-Higgs (YMH) equations for the gauge group U(2). Thus our results can be rephrased as the corresponding statements about the U(2)-YMH equations.












This page was built for publication: Instability of electroweak homogeneous vacua in strong magnetic fields

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6508130)