  The spinning electromagnetic universe, known also as the Rotating
Bertotti-Robinson(RBR) spacetime is considered as a model to represent our
cosmos. The model derives from different physical considerations, such as
colliding waves, throat region, and near horizon geometry of the Kerr-Newman
black hole. Our interest is whether such a singularity-free spinning cosmology
gives rise to a natural direction of flow, a 'chirality' for charged particles.
Homochiral structures are known to be crucial for biology to start. Our concern
here is cosmology rather than biology, but as in biology, the stable structures
in cosmology may also rely on homochiral elements. We show the occurrence of
closed timelike curves a 'la' G{\"o}del. Such curves, however, seem possible
only at localized cell structures, not at large scales, but according to our
prescription of near horizon geometry, they arise in the vicinity of any
charged, spinning black hole.
