Geodesics of Robertson-Walker Universes

Physics

Scientific paper

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Scientific paper

The complete set of geodesics is obtained for Robertson-Walker universes with arbitrary R(t), from those geodesics whose spatial projections pass through the origin, by inducing a translation of origin through the rotation of a hypersphere whose stereographic projections form the space sections. The results are applied to the calculation, in a Milne universe, of the angular displacement of a particle initially projected at high velocity accross the line of sight. This displacement proves to be bounded, the upper bound being attained reasonably fast, on a cosmic time scale.

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