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      Wheeler-DeWitt equation and Lie symmetries in Bianchi scalar-field cosmology

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          Abstract

          Lie symmetries are discussed for the Wheeler-De Witt equation in Bianchi Class A cosmologies. In particular, we consider General Relativity, minimally coupled scalar field gravity and Hybrid Gravity as paradigmatic examples of the approach. Several invariant solutions are determined and classified according to the form of the scalar field potential. The approach gives rise to a suitable method to select classical solutions and it is based on the first principle of the existence of symmetries.

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          Inhomogeneous cosmologies with cosmological constant

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            Spatially Homogeneous and Euclidean Cosmological Models with Shear

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              Metric-Palatini gravity unifying local constraints and late-time cosmic acceleration

              We present a novel approach to modified theories of gravity that consists of adding to the Einstein-Hilbert Lagrangian an f(R) term constructed a la Palatini. Using the respective dynamically equivalent scalar-tensor representation, we show that the theory can pass the Solar System observational constraints even if the scalar field is very light. This implies the existence of a long-range scalar field, which is able to modify the cosmological and galactic dynamics, but leaves the Solar System unaffected. We also verify the absence of instabilities in perturbations and provide explicit models which are consistent with local tests and lead to the late-time cosmic acceleration.
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                Author and article information

                Journal
                2016-01-25
                Article
                10.1140/epjc/s10052-016-4087-8
                1601.06528
                4c6bc0df-7e2b-4707-bfc2-70e8f5745284

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                17 pages
                gr-qc hep-th

                General relativity & Quantum cosmology,High energy & Particle physics
                General relativity & Quantum cosmology, High energy & Particle physics

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