Rainbow universe
arXiv:gr-qc/0609129 · doi:10.1088/1475-7516/2007/08/017
Abstract
The formalism of rainbow gravity is studied in a cosmological setting. We consider the very early universe which is radiation dominated. A novel treatment in our paper is to look for an ``averaged'' cosmological metric probed by radiation particles themselves. Taking their cosmological evolution into account, we derive the modified Friedmann-Robertson-Walker(FRW) equations which is a generalization of the solution presented by Magueijo and Smolin. Based on this phenomenological cosmological model we argue that the spacetime curvature has an upper bound such that the cosmological singularity is absent. These modified equations can be treated as effective equations in the semi-classical framework of quantum gravity and its analogy with the one recently proposed in loop quantum cosmology is also discussed.
5 pages
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Cited by in corpus (52)
- The General Very Special Relativity in Finsler Cosmology
- Nonsingular Rainbow Universes
- Black Hole Remnant from Gravity's Rainbow
- Nonsingular Universes in Gauss-Bonnet Gravity's Rainbow
- Modified (A)dS Schwarzschild black holes in Rainbow spacetime
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- Expansion of magnetic neutron stars in an energy (in)dependent spacetime
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- The Big Bounce in Rainbow Universe
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