Rotating ``black holes'' with holes in the horizon
Kerr-Schild solutions of the Einstein-Maxwell field equations, containing semi-infinite axial singular lines, are investigated. It is shown that axial singularities break up the black hole, forming holes in the horizon. As a result, a tubelike region appears which allows matter to escape from the interior without crossing the horizon. It is argued
Burinskii, Alexander et al.
Fecha de publicación:
7
2006