Multimetric extension of the PPN formalism: experimental consistency of repulsive gravity
arXiv:1007.4945 · doi:10.1103/PhysRevD.82.084028
Abstract
Recently we discussed a multimetric gravity theory containing several copies of standard model matter each of which couples to its own metric tensor. This construction contained dark matter sectors interacting repulsively with the visible matter sector, and was shown to lead to cosmological late-time acceleration. In order to test the theory with high-precision experiments within the solar system we here construct a simple extension of the parametrized post-Newtonian (PPN) formalism for multimetric gravitational backgrounds. We show that a simplified version of this extended formalism allows the computation of a subset of the PPN parameters from the linearized field equations. Applying the simplified formalism we find that the PPN parameters of our theory do not agree with the observed values, but we are able to improve the theory so that it becomes consistent with experiments of post-Newtonian gravity and still features its promising cosmological properties.
arXiv comment19 pages, no figures, journal version
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Cited by in corpus (6)
- Post-Newtonian parameter and the deflection of light in ghost-free massive bimetric gravity
- Gauge-invariant approach to the parametrized post-Newtonian formalism
- Parameterized post-Newtonian formalism for multimetric gravity
- xPPN: An implementation of the parametrized post-Newtonian formalism using xAct for Mathematica
- Propagation of gravitational waves in multimetric gravity
- Repulsive gravity induced by a conformally coupled scalar field implies a bouncing radiation-dominated universe