Single-Field Inflation and the Local Ansatz: Distinguishability and Consistency
arXiv:1610.00785 · doi:10.1103/PhysRevD.95.063501
Abstract
The single-field consistency conditions and the local ansatz have played separate but important roles in characterizing the non-Gaussian signatures of single- and multifield inflation respectively. We explore the precise relationship between these two approaches and their predictions. We demonstrate that the predictions of the single-field consistency conditions can never be satisfied by a general local ansatz with deviations necessarily arising at order . This implies that there is, in principle, a minimum difference between single- and (fully local) multifield inflation in observables sensitive to the squeezed limit such as scale-dependent halo bias. We also explore some potential observational implications of the consistency conditions and its relationship to the local ansatz. In particular, we propose a new scheme to test the consistency relations. In analogy with delensing of the cosmic microwave background, one can deproject the coupling of the long wavelength modes with the short wavelength modes and test for residual anomalous coupling.
arXiv comment17 pages
References in corpus (52)
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Weak Gravitational Lensing of the CMB
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- The primordial density perturbation in the curvaton scenario
- Single field consistency relation for the 3-point function
- The linear power spectrum of observed source number counts
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- Constraints on local primordial non-Gaussianity from large scale structure
- What galaxy surveys really measure
- The effect of primordial non-Gaussianity on halo bias
- Reconstruction of lensing from the cosmic microwave background polarization
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- Adiabatic Modes in Cosmology
- On Soft Limits of Inflationary Correlation Functions
- Large-scale clustering of galaxies in general relativity
- Violation of non-Gaussianity consistency relation in a single field inflationary model
- Non-Gaussianities in models with a varying inflaton decay rate
- The Effective Field Theory of Multifield Inflation
- Non-Gaussianity in the modulated reheating scenario
- Conformal consistency relations for single-field inflation
- The Observed Squeezed Limit of Cosmological Three-Point Functions
- Cosmology with the SPHEREX All-Sky Spectral Survey
- Single-Field Consistency Relations of Large Scale Structure
- Delensing CMB Polarization with External Datasets
- Galaxy Bias and non-Linear Structure Formation in General Relativity
- A Single Field Inflation Model with Large Local Non-Gaussianity
- Primordial non-Gaussianity from the large scale structure
- Going beyond the Kaiser redshift-space distortion formula: a full general relativistic account of the effects and their detectability in galaxy clustering
- Testing General Relativity on Horizon Scales and the Primordial non-Gaussianity
- Symmetries and Loops in Inflation
- Signs of Analyticity in Single-Field Inflation
- Disentangling non-Gaussianity, bias and GR effects in the galaxy distribution
- A model with cosmological Bell inequalities
- A Note on the Consistency Condition of Primordial Fluctuations
- One-particle-irreducible consistency relations for cosmological perturbations
- On Squeezed Limits in Single-Field Inflation - Part I
- On Separate Universes
- CMB Delensing Beyond the B Modes
- Stochastic Bias from Non-Gaussian Initial Conditions
- Consistently violating the non-Gaussian consistency relation
- A universal bound on N-point correlations from inflation
- Designing an Inflation Galaxy Survey: how to measure using scale-dependent galaxy bias
- B-modes and the Nature of Inflation
- Constraining primordial non-Gaussianity via a multitracer technique with surveys by Euclid and Square Kilometre Array
- Using Large Scale Structure to test Multifield Inflation
- Is There Scale-Dependent Bias in Single-Field Inflation?
- Statistical Naturalness and non-Gaussianity in a Finite Universe
- Consistency Relations for Non-Gaussianity
- Non-Gaussian Mode Coupling and the Statistical Cosmological Principle
- The consistency condition for the three-point function in dissipative single-clock inflation
- Loop corrections and a new test of inflation
- Effective Theory of Squeezed Correlation Functions
Cited by in corpus (7)
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure
- The Power of Locality: Primordial Non-Gaussianity at the Map Level
- Vanishing of local non-Gaussianity in canonical single field inflation
- Non-Gaussian CMB and LSS statistics beyond polyspectra
- Constraining using the Large-Scale Modulation of Small-Scale Statistics
- Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects