On the space of non-Gaussian fields with single-clock bispectra
arXiv:1605.07206 · doi:10.1103/PhysRevD.94.043510
Abstract
We develop a mathematical construction of non-Gaussian fields whose bispectra satisfy the single-clock inflation consistency relation. At the same order that our basis for bispectra recovers the two simplest single clock templates, we also find a third orthogonal template which has the single clock squeezed limit, peaks in folded configurations, and has very small coupling in the equilateral limit. We explore the map between templates and operators in a very general Lagrangian for single-clock fluctuations and find no significant overlap between the new template and models in the literature. We comment on the physical implications of this conclusion. Our findings add support for the idea that both theory and data driven considerations will be best served if next generation non-Gaussianity constraints are made in a basis that uses the degree of coupling between long and short wavelength modes as an organizing principle.
14 pages, 6 figures
References in corpus (59)
- Generating the curvature perturbation without an inflaton
- The Effective Field Theory of Inflation
- Adiabatic CMB perturbations in pre-big bang string cosmology
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- Nongaussian Isocurvature Perturbations from Inflation
- Single field consistency relation for the 3-point function
- Quasi-Single Field Inflation and Non-Gaussianities
- A new mechanism for generating density perturbations from inflation
- The shape of non-Gaussianities
- Non-Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data
- On Soft Limits of Inflationary Correlation Functions
- Generation and Characterization of Large Non-Gaussianities in Single Field Inflation
- Galileon inflation
- Non-Gaussianities in models with a varying inflaton decay rate
- The Effective Field Theory of Multifield Inflation
- On the consistency relation of the 3-point function in single field inflation
- Features and New Physical Scales in Primordial Observables: Theory and Observation
- Conformal consistency relations for single-field inflation
- Resonant Non-Gaussianity
- The shape of primordial non-Gaussianity and the CMB bispectrum
- Signatures of Initial State Modifications on Bispectrum Statistics
- The anisotropic power spectrum and bispectrum in the f(phi) F^2 mechanism
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- An Infinite Set of Ward Identities for Adiabatic Modes in Cosmology
- Galilean symmetry in the effective theory of inflation: new shapes of non-Gaussianity
- Dissipative effects in the Effective Field Theory of Inflation
- Folded Resonant Non-Gaussianity in General Single Field Inflation
- Effective field theory and non-Gaussianity from general inflationary states
- Large non-Gaussianities in the Effective Field Theory Approach to Single-Field Inflation: the Bispectrum
- A Note on the Consistency Condition of Primordial Fluctuations
- One-particle-irreducible consistency relations for cosmological perturbations
- (Small) Resonant non-Gaussianities: Signatures of a Discrete Shift Symmetry in the Effective Field Theory of Inflation
- On Separate Universes
- Bispectrum signatures of a modified vacuum in single field inflation with a small speed of sound
- Conformal Fermi Coordinates
- The long-short wavelength mode coupling tightens primordial black hole constraints
- A non-Gaussian landscape
- Statistical Naturalness and non-Gaussianity in a Finite Universe
- Large-scale anomalies in the cosmic microwave background as signatures of non-Gaussianity
- Oscillations in the Primordial Bispectrum: Mode Expansion
- Multiple Soft Limits of Cosmological Correlation Functions
- Double Soft Limits of Cosmological Correlations
- The squeezed limit of the bispectrum in multi-field inflation
- Cosmic variance in inflation with two light scalars
- Non-Gaussianity from Axion Monodromy Inflation
- Non-Gaussian Mode Coupling and the Statistical Cosmological Principle
- The consistency condition for the three-point function in dissipative single-clock inflation
- Statistics of Anisotropies in Inflation with Spectator Vector Fields
- Cosmic Variance of the Spectral Index from Mode Coupling
- Implications of the Planck bispectrum constraints for the primordial trispectrum
- Non-Gaussian Shape Recognition
- Super cosmic variance from mode-coupling: A worked example
- Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
- Non-local bispectra from super cosmic variance
- Local Observables in a Landscape of Infrared Gauge Modes
- Resonant non-Gaussianity with equilateral properties
- New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data
- Looking for non-Gaussianity in all the right places: A new basis for non-separable bispectra
- Optimal bispectrum constraints on single-field models of inflation