Abstract
A sense in which flat space-time can be recovered as a limit of the newly discovered Hauser space-times (see Phys. Rev. Lett., vol.33, p.1112 of 1974) is discussed. Thus a fairly complete analysis of the symmetries of these space-times, together with the geometry of their linearized principal congruences and Weyl curvature tensors can be made. Unfortunately the Hauser space-times are not asymptotically flat and cannot therefore be regarded as describing gravitational radiation from an isolated system.

This publication has 7 references indexed in Scilit: