Minimal cut-off vacuum state constraints from CMB bispectrum statistics
arXiv:1009.5660 · doi:10.1103/PhysRevD.83.043520
Abstract
In this short note we translate the best available observational bounds on the CMB bispectrum amplitudes into constraints on a specific scale-invariant New Physics Hypersurface (NPH) model of vacuum state modifications, as first proposed by Danielsson, in general models of single-field inflation. As compared to the power spectrum the bispectrum constraints are less ambiguous and provide an interesting upper bound on the cut-off scale in general models of single-field inflation with a small speed of sound. This upper bound is incompatible with the power spectrum constraint for most of the parameter domain, leaving very little room for minimal cut-off vacuum state modifications in general single-field models with a small speed of sound.
9 pages, 1 figure
References in corpus (9)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Enhanced Non-Gaussianity from Excited Initial States
- The shape of primordial non-Gaussianity and the CMB bispectrum
- Optimal limits on f_{NL}^{local} from WMAP 5-year data
- Folded Resonant Non-Gaussianity in General Single Field Inflation
- Oscillations in the inflaton potential?
- Quantum modes in DBI inflation: exact solutions and constraints from vacuum selection