Mathematics
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978gregr...9..763b&link_type=abstract
General Relativity and Gravitation, vol. 9, Sept. 1978, p. 763-771.
Mathematics
3
Astronomical Models, Relativity, Space-Time Functions, Symmetry, Torsion, Universe, Cosmology, Equations Of Motion, Singularity (Mathematics), Vorticity
Scientific paper
It is shown that a homogeneous and isotropic universe possessing totally antisymmetric torsion is possible and that the equation of motion in this case leads to predictions which parallel those of the Einstein case. The concept of a symmetric space is considered which allows the space to be endowed with torsion, and a three-dimensional space that is homogeneous and isotropic at every point is defined in which the totally antisymmetric torsion is required to be form invariant on a manifold that has the maximum number of linearly independent Killing vectors. A full spacetime metric for a four-dimensional space that is split up into a family of three-dimensional maximally symmetric hypersurfaces orthogonal to the timelike congruence is derived which leads to a closed universe and is identical to the Robertson-Walker metric of Einstein relativity. An equation of motion is obtained for which the behavior of the universe is cyclic and similar to that predicted in the case of zero torsion.
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