Non-Gaussian Inflationary Perturbations from the dS/CFT Correspondence
arXiv:astro-ph/0604209 · doi:10.1088/1475-7516/2006/06/001
Abstract
We use the dS/CFT correspondence and bulk gravity to predict the form of the renormalized holographic three-point correlation function of the operator which is dual to the inflaton field perturbation during single-field, slow-roll inflation. Using Maldcaena's formulation of the correspondence, this correlator can be related to the three-point function of the curvature perturbation generated during single-field inflation, and we find exact agreement with previous bulk QFT calculations. This provides a consistency check on existing derivations of the non-Gaussianity from single-field inflation and also yields insight into the nature of the dS/CFT correspondence. As a result of our calculation, we obtain the properly renormalized dS/CFT one-point function, including boundary contributions where derivative interactions are present in the bulk. In principle, our method may be employed to derive the n-point correlators of the inflationary curvature perturbation within the context of (n-1)th-order perturbation theory, rather than nth-order theory as in conventional approaches.
23 pages, uses iopart.cls. Replaced with version accepted by JCAP; some clarifications in the introduction, and references added
References in corpus (10)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Angular Trispectrum of CMB Temperature Anisotropy from Primordial Non-Gaussianity with the Full Radiation Transfer Function
- Non-gaussianity from the second-order cosmological perturbation
- Non-Gaussianity from Preheating
- Non-gaussianity and cosmic uncertainty in curvaton-type models
- A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
- Seed perturbations for primordial magnetic fields from MSSM flat directions
- Non-Gaussianity in braneworld and tachyon inflation
- A Statistically Robust 3-Sigma Detection of Non-Gaussianity in the WMAP Data Using Hot and Cold Spots
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- Consistency condition for inflation from (broken) conformal symmetry
- Cosmological 3-point correlators from holography
- Predictions for Nongaussianity from Nonlocal Inflation
- Non-Gaussian corrections to the probability distribution of the curvature perturbation from inflation
- Multi-field inflation from holography
- Non-Gaussian inflationary shapes in theories beyond Horndeski
- Renormalisation of IR divergences and holography in de Sitter
- Proving the absence of large one-loop corrections to the power spectrum of curvature perturbations in transient ultra-slow-roll inflation within the path-integral approach
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- Improvement of energy-momentum tensor and non-Gaussianities in holographic cosmology
- Absence of one-loop effects on large scales from small scales in non-slow-roll dynamics
- Holographic non-Gaussianities in general single-field inflation
- Cosmology at the boundary of de Sitter using the dS/QFT correspondence
- Holographic Entanglement Entropy in the FLRW Universe
- Unitarity at Infinity and Topological Holography
- Effects of high-order operators in non-relativistic Lifshitz holography
- Cosmological singleton gravity theory and dS/LCFT correspondence
- Cosmological three-coupled scalar theory for the dS/LCFT correspondence