Breaking of Spatial Diffeomorphism Invariance, Inflation and the Spectrum of Cosmological Perturbations
arXiv:1506.00896 · doi:10.1088/1475-7516/2015/10/009
Abstract
Standard inflationary models yield a characteristic signature of a primordial power spectrum with a red tensor and scalar tilt. Nevertheless, Cannone et al recently suggested that, by breaking the assumption of spatial diffeomorphism invariance in the context of the effective field theory of inflation, a blue tensor spectrum can be achieved without violating the Null Energy Condition. In this context, we explore in which cases a blue tensor tilt can be obtained along with a red tilt in the scalar spectrum. Ultimately, we analyze under which conditions this model can reproduce the specific consistency relation of String Gas Cosmology.
6 pages
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- Primordial black holes as a novel probe of primordial gravitational waves. II: Detailed analysis
- Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
- Higher derivative scalar-tensor theory through a non-dynamical scalar field
- Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
- Self-gravitating -media
- Charged Lifshitz black holes from general covariance breaking
- Gravitational waves in a cyclic Universe: resilience through cycles and vacuum state