Physics defines rest mass of an object as that measured by a relatively motionless observer. In this sense rest mass in no way implies absoluteness. On the other hand, since absolute motion is almost impossible to measure, the best surmise is that rest mass indicates parallel displacements of equal absolute magnitudes between object and observer. However, in a universe of positive or negative curvature, parallel displacements are impossible without dimensional extension. Fortunately, these curvatures could be demonstrated effectively within localized massive objects such as stars, galaxies, and black holes. Globally, the cosmological flatness problem would not go away. This calls for a more plausible spatiotemporal theory of perfect symmetry.


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