Radiation-dominated area metric cosmology
arXiv:0705.4656 · doi:10.1088/1475-7516/2007/12/013
Abstract
We provide further crucial support for a refined, area metric structure of spacetime. Based on the solution of conceptual issues, such as the consistent coupling of fermions and the covariant identification of radiation fields on area metric backgrounds, we show that the radiation-dominated epoch of area metric cosmology is equivalent to that epoch in standard Einstein cosmology. This ensures, in particular, successful nucleosynthesis. This surprising result complements the previously derived prediction of a small late-time acceleration of an area metric universe.
23 pages, no figures; references added
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Cited by in corpus (10)
- How to Distinguish Dark Energy and Modified Gravity?
- Causal structure and algebraic classification of area metric spacetimes in four dimensions
- Birefringence in pseudo-Finsler spacetimes
- Pseudo-Finslerian spacetimes and multi-refringence
- Propagation of light in area metric backgrounds
- Maxwell's equations in Minkowski's world: their premetric generalization and the electromagnetic energy-momentum tensor
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- Brans-Dicke geometry
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- Geometry of Area Without Length