Autoparallel vs. Geodesic Trajectories in a Model of Torsion Gravity
We consider a parametrized torsion gravity model for Riemann–Cartan geometry around a rotating axisymmetric massive body. In this model, the source of torsion is given by a circulating vector potential following the celestial parallels around the rotating object. Ours is a variant of the Mao, Tegmar...
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| Format: | Article |
| Language: | English |
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MDPI AG
2015-11-01
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| Series: | Universe |
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| Online Access: | http://www.mdpi.com/2218-1997/1/3/422 |