GENERALIZED MAGNETIC UNIVERSE SOLUTIONS

We apply the techniques that have been developed over the last few decades for generating nontrivially new solutions of the Einstein-Maxwell equations from seed solutions for simple spacetimes. The simple seed spacetime that we choose is the ''magnetic universe'' to which we apply the Ehlers transformation. Three interesting nonsingular metrics are generated. Two of these may be described as ''rotating magnetic universes'' and the third as an ''evolving magnetic universe.'' Each is causally complete, in that all timelike and lightlike geodesics do not end in a finite time or affine parameter. We also give the electromagnetic field in each case. For the two rotating stationary cases we give the projection with respect to a stationary observer of the electromagnetic field into electric and magnetic components.