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arXiv · gr-qc/0510055

3D gravity and non-linear cosmology

F. P. Devecchi·M. L. Froehlich
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Abstract

By the inclusion of an additional term, non-linear in the scalar curvature $R$, it is tested if dark energy could rise as a geometrical effect in 3D gravitational formulations. We investigate a cosmological fluid obeying a non-polytropic equation of state (the van der Waals equation) that is used to construct the energy-momentum tensor of the sources, representing the hypothetical inflaton in gravitational interaction with a matter contribution. Following the evolution in time of the scale factor, its acceleration, and the energy densities of constituents it is possible to construct the description of an inflationary 3D universe, followed by a matter dominated era. For later times it is verified that, under certain conditions, the non-linear term in $R$ can generate the old 3D universe in accelerated expansion, where the ordinary matter is represented by the barotropic limit of the van der Waals constituent.

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F. P. Devecchi, M. L. Froehlich. 2005-10-11. 3D gravity and non-linear cosmology. https://doi.org/10.1142/s0217732306018974

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