Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure
arXiv:1803.11539 · doi:10.1103/PhysRevLett.121.101301
Abstract
We develop a new method to constraint primordial non-Gaussianities of the local kind using unclustered tracers of the Large Scale Structure. We show that in the limit of low noise, zero bias tracers yield large improvement over standard methods, mostly due to vanishing sampling variance. We propose a simple technique to construct such a tracer, using environmental information obtained from the original sample, and validate our method with N-body simulations. Our results indicate that can be reached using only information on a single tracer of sufficiently high number density.
arXiv comment6 pages, 3 figures
References in corpus (49)
- Planck 2015 results. XIII. Cosmological parameters
- The cosmological simulation code GADGET-2
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Generating the curvature perturbation without an inflaton
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Cosmology and fundamental physics with the Euclid satellite
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- Nongaussian Isocurvature Perturbations from Inflation
- Single field consistency relation for the 3-point function
- A new mechanism for generating density perturbations from inflation
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- A hierarchy of voids: Much ado about nothing
- Constraints on local primordial non-Gaussianity from large scale structure
- Measuring cosmological parameters with galaxy surveys
- Non-Gaussianity of the primordial perturbation in the curvaton model
- The effect of primordial non-Gaussianity on halo bias
- Measuring primordial non-gaussianity without cosmic variance
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics
- Non-Gaussianities in models with a varying inflaton decay rate
- Scale-dependent bias induced by local non-Gaussianity: A comparison to N-body simulations
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- Halo Stochasticity from Exclusion and non-linear Clustering
- Large scale bias and stochasticity of halos and dark matter
- Minimizing the stochasticity of halos in large-scale structure surveys
- The Clustering of Galaxies in SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: Constraints on Primordial Non-Gaussianity
- Primordial non-Gaussianity from the large scale structure
- Constraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys
- Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
- Halo assembly bias and the tidal anisotropy of the local halo environment
- Hunting down horizon-scale effects with multi-wavelength surveys
- Cosmology with Void-Galaxy Correlations
- Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
- Cosmology on Ultralarge Scales with Intensity Mapping of the Neutral Hydrogen 21 cm Emission: Limits on Primordial Non-Gaussianity
- Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
- Linear redshift space distortions for cosmic voids based on galaxies in redshift space
- Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
- Designing an Inflation Galaxy Survey: how to measure using scale-dependent galaxy bias
- Extending the modeling of the anisotropic galaxy power spectrum to
- Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
- Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest
- Non-Gaussian halo assembly bias
- The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- Systematic effects in large-scale angular power spectra of photometric quasars and implications for constraining primordial nongaussianity
- Using Large Scale Structure to test Multifield Inflation
- Biasing and the search for primordial non-Gaussianity beyond the local type
- Dependence of halo bias on mass and environment
- The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
- What determines large scale galaxy clustering: halo mass or local density?
- Single-Field Inflation and the Local Ansatz: Distinguishability and Consistency
Cited by in corpus (23)
- Redshift-weighted constraints on primordial non-Gaussianity from the clustering of the eBOSS DR14 quasars in Fourier space
- Nearest Neighbor distributions: new statistical measures for cosmological clustering
- On the impact of galaxy bias uncertainties on primordial non-Gaussianity constraints
- The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
- Imprints of Oscillatory Bispectra on Galaxy Clustering
- Constraint of Void Bias on Primordial non-Gaussianity
- Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
- Non-Gaussianity Constraints using Future Radio Continuum Surveys and the Multi-Tracer Technique
- Weighing neutrinos with the halo environment
- Relativistic cosmological large scale structures at one-loop
- Local Primordial Non-Gaussianities and Super-Sample Variance
- Neutrino Mass Signatures in the Galaxy Bispectrum
- Cosmology in nonlocal gravity
- Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field
- Shot noise in multi-tracer constraints on and relativistic projections: Power Spectrum
- Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
- The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
- Supergravity, -attractors and primordial non-Gaussianity
- Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
- Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept
- Non-Gaussianities in generalized non-local -like inflation
- Quijote PNG: The information content of the halo power spectrum and bispectrum
- Unclustered tracers remain unclustered: the lack of primordial non-Gaussianity response of bias-zero tracers