Static black hole solutions without rotational symmetry
Static black hole solutions without rotational symmetry
We construct static black hole solutions that have no rotational symmetry. These arise in theories (including the standard electroweak model) that contain charged vector mesons with mass m\ensuremath{\ne}0. In such theories, a magnetically charged Reissner-Nordstr\"om black hole with horizon radius less than a critical value of order ${\mathit{m}}^{\mathrm{\ensuremath{-}}1}$ is classically …