Vector inflation by kinetic coupled gravity
arXiv:1401.1280 · doi:10.1142/S0218271814500692
Abstract
Vector inflation is a newly established model where inflation is driven by non-minimally coupled massive vector fields with a potential term. This model is similar to the model of chaotic inflation with scalar fields, except that for vector fields the isotropy of expansion is achieved either by considering a triplet of orthogonal vector fields or randomly oriented independent vector fields. We introduce a new version of vector inflation where the vector field has no potential term but is non-minimally coupled to gravity through the kinetic term. The non-minimal coupling is established by introducing the Einstein tensor besides the metric tensor within the kinetic term of the vector field.
9 pages
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Cited by in corpus (10)
- Inflation with an antisymmetric tensor field
- Inflation driven by massive vector fields with derivative self-interactions
- Avoiding instabilities in antisymmetric tensor field driven inflation
- Slow-roll inflation from massive vector fields non-minimally coupled to gravity
- Gravitational waves from inflation with antisymmetric tensor field
- Inflation with antisymmetric tensor field: new candidates
- Inflation using a triplet of Antisymmetric tensor fields
- Power-law Bianchi type I inflation with multiple vector fields
- Covariant Quantum Gravitational Corrections to Scalar and Tensor Field Models
- Non-minimal kinetic coupled gravity: inflation on the Warped DGP brane