A numerical study of non-gaussianity in the curvaton scenario
arXiv:astro-ph/0604387 · doi:10.1088/1475-7516/2006/09/008
Abstract
We study the curvaton scenario using gauge-invariant second order perturbation theory and solving the governing equations numerically. Focusing on large scales we calculate the non-linearity parameter f_nl in the two-fluid curvaton model and compare our results with previous analytical studies employing the sudden decay approximation. We find good agreement of the two approaches for large curvaton energy densities at curvaton decay, Omega_dec, but significant differences of up to 10 percent for small Omega_dec.
arXiv comment15 pages, 9 figures, some in colour; v2: references added, typos corrected, section on curvaton evolution added; v3: typos corrected, corresponds to journal version
References in corpus (40)
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Generating the curvature perturbation without an inflaton
- Non-Gaussianity from Inflation: Theory and Observations
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
- Adiabatic CMB perturbations in pre-big bang string cosmology
- A new approach to the evolution of cosmological perturbations on large scales
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- A general proof of the conservation of the curvature perturbation
- The primordial density perturbation in the curvaton scenario
- Second-Order Cosmological Perturbations from Inflation
- The inflationary prediction for primordial non-gaussianity
- Super-Horizon Scale Dynamics of Multi-Scalar Inflation
- Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
- On the Back Reaction Problem for Gravitational Perturbations
- Primordial non-gaussianities from multiple-field inflation
- Non-Gaussianity in multi-field inflation
- On Non-Gaussianity in the Curvaton Scenario
- Second-order Perturbations of the Friedmann World Model
- Non-Gaussianity from Inflation
- Large-scale curvature and entropy perturbations for multiple interacting fluids
- Evolution of second-order cosmological perturbations
- Conserved cosmological perturbations
- Cosmic Density Perturbations from Late-Decaying Scalar Condensations
- Inflationary models inducing non-Gaussian metric fluctuations
- Non-gaussianity from the second-order cosmological perturbation
- Non-Gaussianity in Curvaton Models with Nearly Quadratic Potential
- Conserved non-linear quantities in cosmology
- Adiabatic and entropy perturbations with interacting fluids and fields
- Gauge-Invariant Temperature Anisotropies and Primordial Non-Gaussianity
- Non-gaussianity and cosmic uncertainty in curvaton-type models
- Evolution of Second-Order Cosmological Perturbations and Non-Gaussianity
- Can the curvaton paradigm accommodate a low inflation scale?
- Non-Gaussian perturbations in hybrid inflation
- Relativistic second-order perturbations of nonzero-Λflat cosmological models and CMB anisotropies
- Gauge Invariant Variables in Two-Parameter Nonlinear Perturbations
- Gauge-invariant perturbations at second order: multiple scalar fields on large scales
- Non-linear inflationary perturbations
- Simple route to non-Gaussianity in inflation
- Curvature and isocurvature perturbations in a three-fluid model of curvaton decay
Cited by in corpus (109)
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity
- Non-Gaussianity of the primordial perturbation in the curvaton model
- Enhanced Non-Gaussianity from Excited Initial States
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Non-Gaussianity in the modulated reheating scenario
- Signatures of Initial State Modifications on Bispectrum Statistics
- A Hemispherical Power Asymmetry from Inflation
- Review of local non-Gaussianity from multi-field inflation
- Non-linear isocurvature perturbations and non-Gaussianities
- Gravitational waves from an early matter era
- Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics, and comparison with N-body simulations
- Conditions for large non-Gaussianity in two-field slow-roll inflation
- Scale-dependent non-Gaussianity probes inflationary physics
- Multiple field inflation
- One-loop corrections to a scalar field during inflation
- Signatures of Non-Gaussianity in the Curvaton Model
- Primordial non-Gaussianities in general modified gravitational models of inflation
- Non-Gaussianity beyond slow roll in multi-field inflation
- Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
- Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays
- Primordial Non-Gaussianity in Multi-Scalar Slow-Roll Inflation
- Curvaton with Polynomial Potential
- Large non-Gaussianity from two-component hybrid inflation
- On the full trispectrum in single field DBI-inflation
- Non-Gaussianity from isocurvature perturbations
- Large Nongaussianity from Nonlocal Inflation
- On Classification of Models of Large Local-Type Non-Gaussianity
- On Features and Nongaussianity from Inflationary Particle Production
- Non-Gaussianity in Two-Field Inflation
- Curvaton Dynamics and the Non-Linearity Parameters in Curvaton Model
- Shapes of primordial non-Gaussianities in the Horndeski's most general scalar-tensor theories
- Diagrammatic approach to non-Gaussianity from inflation
- Non-gaussianity of inflationary field perturbations from the field equation
- A General Analysis of Non-Gaussianity from Isocurvature Perturbations
- Encyclopaedia Curvatonis
- Primordial non-Gaussianity from two curvaton decays
- On the full quantum trispectrum in multi-field DBI inflation
- Isocurvature, non-gaussianity and the curvaton model
- Lorentz boost and non-Gaussianity in multi-field DBI-inflation
- Predictions for Nongaussianity from Nonlocal Inflation
- The Subdominant Curvaton
- Priomordial non-Gaussian features from DBI Galileon inflation
- Primordial Black Hole Formation in Non-Minimal Curvaton Scenario
- Limits on Isocurvature Perturbations from Non-Gaussianity in WMAP Temperature Anisotropies
- Scale-dependence of Non-Gaussianity in the Curvaton Model
- Hilltop Non-Gaussianity
- Nongaussianity from Particle Production During Inflation
- Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
- Non-Gaussianity from the hybrid potential
- Non-Gaussianity from Symmetry
- Primordial Non-Gaussianities from the Trispectra in Multiple Field Inflationary Models
- Non-Gaussianity from resonant curvaton decay
- A not so short note on the Klein-Gordon equation at second order
- Gravitational Wave Background and Non-Gaussianity as a Probe of the Curvaton Scenario
- Non-Gaussianity in single field models without slow-roll
- N-vaton
- Strongly scale-dependent polyspectra from curvaton self-interactions
- Path Integral for Inflationary Perturbations
- Non-Gaussianity of superhorizon curvature perturbations beyond N formalism
- Reheating, Multifield Inflation and the Fate of the Primordial Observables
- Parametric Decay of the Curvaton
- On Non-Gaussianities in Multi-Field Inflation (N fields): Bi- and Tri-spectra beyond Slow-Roll
- Non-Gaussianity from Isocurvature Perturbations : Analysis of Trispectrum
- Trispectrum from Ghost Inflation
- Primordial Non-Gaussianity in Models with Dark Matter Isocurvature Fluctuations
- Effect of Background Evolution on the Curvaton Non-Gaussianity
- Growth of curvature perturbations for PBH formation \& detectable GWs in non-minimal curvaton scenario revisited
- Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
- Non-Gaussianities of Single Field Inflation with Non-minimal Coupling
- Constraining Curvatonic Reheating
- Non-Gaussianity and Gravitational Waves from Quadratic and Self-interacting Curvaton
- General analytic predictions of two-field inflation and perturbative reheating
- Bispectra from two-field inflation using the long-wavelength formalism
- Measuring the duration of inflation with the curvaton
- Can Standard Model Higgs Seed the Formation of Structures in Our Universe?
- Optimizing future experimental probes of inflation
- Density Fluctuations in Thermal Inflation and Non-Gaussianity
- Anisotropies in Scalar-Induced Gravitational-Wave Background from Inflaton-Curvaton Mixed Scenario with Sound Speed Resonance
- Non-Gaussianity in multiple three-form field inflation
- Primordial curvature perturbation during and at the end of multi-field inflation
- Non-Gaussianity in three fluid curvaton model
- Gravitino Dark Matter and Non-Gaussianity
- Non-linear Preheating with Scalar Metric Perturbations
- Probing a panoply of curvaton-decay scenarios using CMB data
- Modulated decay in the multi-component Universe
- Influence of Reheating on the Trispectrum and its Scale Dependence
- Nonlinear superhorizon perturbations of non-canonical scalar field
- Curvaton and the inhomogeneous end of inflation
- How the curvaton scenario, modulated reheating and an inhomogeneous end of inflation are related
- Nonlinear curvature perturbations in an exactly soluble model of multi-component slow-roll inflation
- What Planck does not tell us about inflation
- On primordial trispectrum from exchanging scalar modes in general multiple field inflationary models
- Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
- Non-Gaussianity and gravitational wave background in curvaton with a double well potential
- Hemispherical Power Asymmetry of the Cosmic Microwave Background from a Remnant of a pre-Inflationary Topological Defect
- Particle Production during Inflation in Light of PLANCK
- New Anisotropic Exact Solution in Multifield Cosmology
- Resolving primordial physics through correlated signatures
- Thermal Effects and Sudden Decay Approximation in the Curvaton Scenario
- Affleck-Dine baryogenesis with modulated reheating
- The Effect of Curvaton Decay on the Primordial Power Spectrum
- Cosmic Microwave Background Dipole Asymmetry could be explained by Axion Monodromy Cosmic Strings
- Primordial black holes from the ultraslow-roll phase in the inflaton--curvaton mixed field inflation
- Primordial black holes from a curvaton: the role of bimodal distributions
- Large non-Gaussianity generated after D-term Inflation by Right-Handed Sneutrino Curvaton
- A Proposal for Constraining Initial Vacuum by CMB
- Curvaton decay into relativistic matter
- Non-Gaussianity after many-field reheating