  We construct stationary solutions to the Einstein-Maxwell-current system by
using the Sasakian manifold for the three-dimensional space. Both the magnetic
field and the electric current in the solution are specified by the contact
form of the Sasakian manifold. The solutions contain an arbitrary function that
describes inhomogeneity of the number density of the charged particles, and the
function determines the curvature of the space.

General Relativity and Quantum Cosmology;Differential Geometry