The cosmology of the nonsymmetric theory of gravitation
arXiv:astro-ph/0503289 · doi:10.1016/j.physletb.2006.03.019
Abstract
We show that during cosmological inflation the nonsymmetric metric tensor theory of gravitation develops a spectrum which is potentially observable by cosmic microwave background observations, and may be the most sensitive probe of the scale of cosmic inflation.
arXiv comment10 pages, 2 figures. The improved version to be published in Phys. Lett. B. Note change in authors
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- Nonholonomic Ricci Flows, Exact Solutions in Gravity, and Symmetric and Nonsymmetric Metrics
- Instabilities in the nonsymmetric theory of gravitation
- Problems and hopes in nonsymmetric gravity
- Probing the String Winding Sector
- Hermitian Gravity and Cosmology
- Einstein Gravity, Lagrange-Finsler Geometry, and Nonsymmetric Metrics
- Vacuum properties of nonsymmetric gravity in de Sitter space
- Gravitational waves from inflation with antisymmetric tensor field
- Nonassociative geometry of nonholonomic phase spaces with star R-flux string deformations and (non) symmetric metrics
- Inflation with antisymmetric tensor field: new candidates
- Inflation using a triplet of Antisymmetric tensor fields
- Scalar and vector modes in inflation with antisymmetric tensor field