Negative spectral index of in the axion-type curvaton model
arXiv:1008.2641 · doi:10.1088/1475-7516/2010/11/026 10.1088/1475-7516/2011/02/E01
Abstract
We derive the spectral index of and its running from isocurvature single field and investigate the curvaton models with a negative spectral index of in detail. In particular, a numerical study of the axion-type curvaton model is illustrated, and we find that the spectral index of is negative and its absolute value is maximized around for the potential . The spectral index of can be for the axion-type curvaton model. A convincing detection of a positive will rule out the axion-type curvaton model. In addition, we also give a general discussion about the detectable parameter space for the curvaton model with a polynomial potential.
arXiv comment14 pages, 2 figures; v2, refs added; version accepted for publication in JCAP
References in corpus (36)
- Generating the curvature perturbation without an inflaton
- A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
- Adiabatic CMB perturbations in pre-big bang string cosmology
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- Equilibrium State of a Massless Self-Interacting Scalar Field in the De Sitter Background
- A general proof of the conservation of the curvature perturbation
- The inflationary prediction for primordial non-gaussianity
- Super-Horizon Scale Dynamics of Multi-Scalar Inflation
- Non-Gaussianity of the primordial perturbation in the curvaton model
- CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
- Non-Gaussianity, Spectral Index and Tensor Modes in Mixed Inflaton and Curvaton Models
- Constraining Running Non-Gaussianity
- Scale-dependent non-Gaussianity probes inflationary physics
- The Curvaton as a Pseudo-Nambu-Goldstone Boson
- Scale dependence of local f_NL
- Signatures of Non-Gaussianity in the Curvaton Model
- Curvaton with Polynomial Potential
- Non-Gaussian Fingerprints of Self-Interacting Curvaton
- Curvaton Dynamics and the Non-Linearity Parameters in Curvaton Model
- A geometric description of the non-Gaussianity generated at the end of multi-field inflation
- Large Non-Gaussianity Implication for Curvaton Scenario
- A General Analysis of Non-Gaussianity from Isocurvature Perturbations
- The Curvature Perturbation in the Axion-type Curvaton Model
- The Subdominant Curvaton
- Scale-dependence of Non-Gaussianity in the Curvaton Model
- Curvaton and QCD Axion in Supersymmetric Theories
- DBI-Curvaton
- Hilltop Non-Gaussianity
- Non-Gaussianity and Baryonic Isocurvature Fluctuations in the Curvaton Scenario
- Non-Gaussianity from Symmetry
- N-vaton
- Primordial Non-Gaussianity in Models with Dark Matter Isocurvature Fluctuations
- Effect of Background Evolution on the Curvaton Non-Gaussianity
- Spectral Index in Curvaton Scenario
- Gravitino Dark Matter and Non-Gaussianity
- Non-Gaussianity with Lagrange Multiplier Field in the Curvaton Scenario
Cited by in corpus (30)
- Constraining primordial non-Gaussianity with future galaxy surveys
- Dynamics of oscillating scalar field in thermal environment
- A generalized local ansatz and its effect on halo bias
- On Classification of Models of Large Local-Type Non-Gaussianity
- The CMB asymmetry from inflation
- Cosmic microwave background anomalies in an open universe
- High-redshift JWST Observations and Primordial Non-Gaussianity
- Testing the Running of non-Gaussianity through the CMB mu-distortion and the Halo Bias
- Strongly Scale-dependent Non-Gaussianity
- Scale-Dependent Non-Gaussianity as a Generalization of the Local Model
- Curvaton with nonminimal derivative coupling to gravity
- Strongly scale-dependent polyspectra from curvaton self-interactions
- Runnings in the Curvaton
- Separable and non-separable multi-field inflation and large non-Gaussianity
- Non-Gaussianity and Gravitational Waves from Quadratic and Self-interacting Curvaton
- General formula for the running of local fNL
- Scale-dependent non-Gaussianity and the CMB Power Asymmetry
- Curvaton with Nonminimal Derivative Coupling to Gravity II: Full Perturbation Analysis
- Isocurvature perturbations in extra radiation
- X-ray Cluster Constraints on Non-Gaussianity
- Can Standard Model Higgs Seed the Formation of Structures in Our Universe?
- G-Curvaton
- Cosmic Variance of the Spectral Index from Mode Coupling
- Tilt and Running of Cosmological Observables in Generalized Single-Field Inflation
- Scale dependence of in N-flation
- Modulated reheating by curvaton
- A weak lensing view on primordial non-Gaussianities
- Scale dependences of local form non-Gaussianity parameters from a DBI isocurvature field
- Spectral index and running of from an isocurvature scalar field
- Generalized local ansatz for scale-dependent primordial non-Gaussianities and future galaxy surveys