Multi-Point Propagators for Non-Gaussian Initial Conditions
arXiv:1006.4656 · doi:10.1103/PhysRevD.82.083507
Abstract
We show here how Renormalized Perturbation Theory (RPT) calculations applied to the quasi-linear growth of the large-scale structure can be carried on in presence of primordial non-Gaussian (PNG) initial conditions. It is explicitly demonstrated that the series reordering scheme proposed in Bernardeau, Crocce and Scoccimarro (2008) is preserved for non-Gaussian initial conditions. This scheme applies to the power spectrum and higher order spectra and is based on a reorganization of the contributing terms into sum of products of multi-point propagators. In case of PNG new contributing terms appear, the importance of which is discussed in the context of current PNG models. The properties of the building blocks of such resummation schemes, the multi-point propagators, are then investigated. It is first remarked that their expressions are left unchanged at one-loop order irrespectively of statistical properties of the initial field. We furthermore show that the high-momemtum limit of each of these propagators can be explicitly computed even for arbitrary initial conditions. They are found to be damped by an exponential cutoff whose expression is directly related to the moment generating function of the one-dimensional displacement field. This extends what had been established for multi-point propagators for Gaussian initial conditions. Numerical forms of the cut-off are shown for the so-called local model of PNG.
16 pages, 6 figures
References in corpus (26)
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
- Renormalized Cosmological Perturbation Theory
- The Three--Point Correlation Function of the Cosmic Microwave Background in Inflationary Models
- Nonlinear Evolution of Baryon Acoustic Oscillations
- Thick gas discs in faint dwarf galaxies
- Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
- Transients from Initial Conditions: A Perturbative Analysis
- Memory of Initial Conditions in Gravitational Clustering
- Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- Resumming Cosmic Perturbations
- Multi-Point Propagators in Cosmological Gravitational Instability
- A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
- Primordial non-Gaussianity from the large scale structure
- Primordial Bispectrum Information from CMB Polarization
- Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
- Signature of Primordial Non-Gaussianity on Matter Power Spectrum
- 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
- Baryonic Acoustic Oscillations via the Renormalization Group
- Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach
- Using the Zeldovich dynamics to test expansion schemes
- Propagators in Lagrangian space
- Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity
Cited by in corpus (31)
- RegPT: Direct and fast calculation of regularized cosmological power spectrum at two-loop order
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
- Peak-Background Split, Renormalization, and Galaxy Clustering
- Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background
- Bias Loop Corrections to the Galaxy Bispectrum
- Constructing Regularized Cosmic Propagators
- MPTbreeze: A fast renormalized perturbative scheme
- Resummed propagators in multi-component cosmic fluids with the eikonal approximation
- Cosmological structure formation with clustering quintessence
- Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
- The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
- Nonlinear Power Spectrum from Resummed Perturbation Theory: a Leap Beyond the BAO Scale
- Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
- Hunting high and low: Disentangling primordial and late-time non-Gaussianity with cosmic densities in spheres
- Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
- Combining perturbation theories with halo models for the matter bispectrum
- Cosmic propagators at two-loop order
- Next-to-leading resummations in cosmological perturbation theory
- Modeling the clustering of dark-matter haloes in resummed perturbation theories
- Cosmological Large-scale Structures beyond Linear Theory in Modified Gravity
- The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
- The nonlinear power spectrum in clustering quintessence cosmologies
- On the importance of nonlinear couplings in large-scale neutrino streams
- Evolution Equation for Non-linear Cosmological Perturbations
- Evolution of dark matter velocity dispersion
- Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
- An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
- Large-k Limit of Multi-Point Propagators in the RG Formalism