Relaxing Constraints on Inflation Models with Curvaton
arXiv:hep-ph/0501007 · doi:10.1103/PhysRevD.72.023502
Abstract
We consider the effects of the curvaton, late-decaying scalar condensation, to observational constraints on inflation models. From current observations of cosmic density fluctuations, severe constraints on some class of inflation models are obtained, in particular, on the chaotic inflation with higher-power monomials, the natural inflation, and the new inflation. We study how the curvaton scenario changes (and relaxes) the constraints on these models.
18 pages, 6 figures
References in corpus (4)
Cited by in corpus (63)
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating
- Non-Gaussianity, Spectral Index and Tensor Modes in Mixed Inflaton and Curvaton Models
- Supergravity based inflation models: a review
- Primordial Black Holes from the inflating curvaton
- Vector Curvaton with varying Kinetic Function
- Extended Slow-Roll Conditions and Rapid-Roll Conditions
- On Classification of Models of Large Local-Type Non-Gaussianity
- Non-Gaussian Fingerprints of Self-Interacting Curvaton
- Encyclopaedia Curvatonis
- The Subdominant Curvaton
- Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations
- Generating primordial features at large scales in two field models of inflation
- Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
- Comprehensive analysis of the simplest curvaton model
- Supergravity inspired Vector Curvaton
- Strongly scale-dependent polyspectra from curvaton self-interactions
- Runnings in the Curvaton
- Primordial Non-Gaussianity in Models with Dark Matter Isocurvature Fluctuations
- Inflation with an extra light scalar field after Planck
- Constraining Curvatonic Reheating
- Non-Gaussianity and Gravitational Waves from Quadratic and Self-interacting Curvaton
- Modular inflation and the orthogonal axion as curvaton
- inflation is not excluded
- Density Perturbations from Modulated Decay of the Curvaton
- Inflation at the TeV scale with a PNGB curvaton
- Optimizing future experimental probes of inflation
- Can Standard Model Higgs Seed the Formation of Structures in Our Universe?
- Density Fluctuations in Thermal Inflation and Non-Gaussianity
- Relaxing inflation models with non-minimal coupling: A general study
- 21 cm Angular Power Spectrum from Minihalos as a Probe of Primordial Spectral Runnings
- Primordial Trispectrum from Isocurvature Fluctuations
- Higher Order Corrections to the Primordial Gravitational Wave Spectrum and its Impact on Parameter Estimates for Inflation
- The minimal curvaton-higgs model
- Constraining isocurvature perturbations with the 21cm emission from minihaloes
- Mixed Inflaton and Spectator Field Models after Planck
- Rescuing Quadratic Inflation
- Probing primordial non-Gaussianity with 21 cm fluctuations from minihalos
- Spectator field models in light of spectral index after Planck
- Non-Gaussianity in the inflating curvaton
- New D-term chaotic inflation in supergravity and leptogenesis
- Violation of slow-roll in non-minimal inflation
- Bayesian evidence of the post-Planck curvaton
- Mixed inflaton and curvaton scenario with sneutrinos
- Modulated reheating by curvaton
- CMB spectral distortions in generic two-field models
- Non-Gaussianity and gravitational wave background in curvaton with a double well potential
- Structure Formation with Two Periods of Inflation: Beyond PLaIn CDM
- Sneutrinos as Mixed Inflaton and Curvaton
- Multi-chaotic inflation with and without spectator field
- The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
- Generating cosmological perturbations with mass variations
- Double inflation via non-minimally coupled spectator
- Thermal Effects and Sudden Decay Approximation in the Curvaton Scenario
- Reheating in Chaotic D-Term Inflation
- Refined Study of Isocurvature Fluctuations in the Curvaton Scenario
- Primordial black holes save inflation
- Large non-Gaussianity generated after D-term Inflation by Right-Handed Sneutrino Curvaton
- The quantum origin of cosmic structure: theory and observations
- Sneutrinos as two inflatons and curvaton and leptogenesis
- Mixed Inflaton and Spectator Field Models: CMB constraints and distortion
- Testing Inflationary Cosmology
- Higher order non-linear parameters with PLANCK