A non-perturbative test of consistency relations and their violation
arXiv:1905.11423 · doi:10.1103/PhysRevD.100.043536
Abstract
In this paper, we verify the large scale structure consistency relations using N-body simulations, including modes in the highly non-linear regime. These relations (pointed out by Kehagias & Riotto and Peloso & Pietroni) follow from the symmetry of the dynamics under a shift of the Newtonian potential by a constant and a linear gradient, and predict the absence of certain poles in the ratio between the (equal time) squeezed bispectrum and power spectrum. The consistency relations, as symmetry statements, are exact, but have not been previously checked beyond the perturbative regime. Our test using N-body simulations not only offers a non-perturbative check, but also serves as a warm-up exercise for applications to observational data. A number of subtleties arise when taking the squeezed limit of the bispectrum--we show how to circumvent or address them. An interesting by-product of our investigation is an explicit demonstration that the linear-gradient symmetry is unaffected by the periodic boundary condition of the simulations. Lastly, we verify using simulations that the consistency relations are violated when the initial conditions are non-gaussian (of the local fNL type). The methodology developed here paves the way for constraining primordial non-gaussianity using large scale structure data, including (numerous) highly non-linear modes that are otherwise hard to interpret and utilize.
arXiv comment10 pages, 5 figures, 1 table
References in corpus (39)
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Single field consistency relation for the 3-point function
- A new mechanism for generating density perturbations from inflation
- How many cosmological parameters?
- Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
- Adiabatic Modes in Cosmology
- On Soft Limits of Inflationary Correlation Functions
- Violation of non-Gaussianity consistency relation in a single field inflationary model
- On the consistency relation of the 3-point function in single field inflation
- Conformal consistency relations for single-field inflation
- Equivalence Principle and the Baryon Acoustic Peak
- The Observed Squeezed Limit of Cosmological Three-Point Functions
- Single-Field Consistency Relations of Large Scale Structure
- Symmetries and Consistency Relations in the Large Scale Structure of the Universe
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- Conformal Symmetries of Adiabatic Modes in Cosmology
- Galilean invariance and the consistency relation for the nonlinear squeezed bispectrum of large scale structure
- An Infinite Set of Ward Identities for Adiabatic Modes in Cosmology
- Operator Product Expansion of Inflationary Correlators and Conformal Symmetry of de Sitter
- Dominance of gauge artifact in the consistency relation for the primordial bispectrum
- One-particle-irreducible consistency relations for cosmological perturbations
- Non-gaussianity and cosmic uncertainty in curvaton-type models
- Single-Field Consistency Relations of Large Scale Structure. Part II: Resummation and Redshift Space
- Single-Field Consistency Relations of Large Scale Structure. Part III: Test of the Equivalence Principle
- Soft Theorems For Shift-Symmetric Cosmologies
- A generalized non-Gaussian consistency relation for single field inflation
- Consequences of Symmetries and Consistency Relations in the Large-Scale Structure of the Universe for Non-local bias and Modified Gravity
- The real shape of non-Gaussianities
- Ward identities and consistency relations for the large scale structure with multiple species
- Soft-Pion Theorems for Large Scale Structure
- Inflationary soft theorems revisited: A generalized consistency relation
- Angular averaged consistency relations of large-scale structures
- A Consistency Relation for the Observed Galaxy Bispectrum and the Local non-Gaussianity from Relativistic Corrections
- Vanishing of local non-Gaussianity in canonical single field inflation
- Equal-time Consistency Relations in the Large-Scale Structure of the Universe
- Testing the equal-time angular-averaged consistency relation of the gravitational dynamics in N-body simulations
- Lagrangian space consistency relation for large scale structure
- Consistency relations for large scale structures with primordial non-Gaussianities
Cited by in corpus (15)
- Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
- Primordial non-Gaussianity from ultra slow-roll Galileon inflation
- The Covariance of Squeezed Bispectrum Configurations
- Consistency relations for large-scale structure in modified gravity and the matter bispectrum
- Large fluctuations and Primordial Black Holes
- New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
- Violation of the consistency relations for large-scale structure with dark energy
- Squeezing out of the matter bispectrum with consistency relations
- Soft theorems for boosts and other time symmetries
- Primordial Black Holes from Effective Field Theory of Stochastic Single Field Inflation at NNNLO
- Unifying attractor and non-attractor models of inflation under a single soft theorem
- Measuring Bias via the Consistency Relations of the Large Scale Structure
- First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
- Model independent measurement of the growth rate from the consistency relations of the LSS
- Constraining using the Large-Scale Modulation of Small-Scale Statistics