On Gödel-type Solution in Rastall's Gravity
arXiv:1407.4322 · doi:10.1142/S021773231550039X
Abstract
Rastall's theory is a generalization of Einstein's equations in which the energy-momentum tensor is not a conserved quantity, its covariant derivative is proportional to the gradient of the Ricci scalar and this fact can be associated with quantum effects in curved space-time. In this work we will go study the Rastall's gravity in the context of the Gödel-type universe.
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Cited by in corpus (11)
- Einstein and Rastall Theories of Gravitation in Comparison
- Thermodynamics of Black Holes in Rastall Gravity
- A connection between Rastall-type and f(R, T) gravities
- Neutral regular black hole solution in generalized Rastall gravity
- Scalar QNMs for higher dimensional black holes surrounded by quintessence in Rastall gravity
- Gödel and Gödel-type universes in Brans-Dicke theory
- The commutator algebra of covariant derivative as general framework for extended gravity. The Rastall theory case and the role of the torsion
- Higher dimensional power-Maxwell charged black holes in Einstein and Rastall gravity
- Source of black bounces in Rastall gravity
- Effects of Rastall parameter on perturbation of dark sectors of the Universe
- Lemaitre-Tolman-Bondi Static Universe in Rastall-like Gravity