Institute for Nuclear Study, University of Tokyo, Tanashi City, Tokyo 188, Japan;Central Research Insitute for Physics, POB 49, H-1525 Budapest 114, Hungary;Department of Physics, University of Pittsburgh, Pittsburgh, PA 15260, USA
Abstract:
The solution of Einstein's vacuum gravitational equations for stationary space—times with a conformally flat 3-space is presented. There is no other solution of this problem than the Ehlers-rotation generalizations of the three conformastat space—times including the Schwarzschild metric.