General Single Field Inflation with Large Positive Non-Gaussianity
arXiv:0801.0040 · doi:10.1088/1475-7516/2008/03/028
Abstract
Recent analysis of the WMAP three year data suggests in the WMAP convention. It is necessary to make sure whether general single field inflation can produce a large positive before turning to other scenarios. We give some examples to generate a large positive in general single field inflation. Our models are different from ghost inflation. Due to the appearance of non-conventional kinetic terms, can be realized in single field inflation.
27 pages, 3 figure; final version published in JCAP
References in corpus (29)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- k-Inflation
- Perturbations in k-inflation
- DBI in the Sky
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Scalar Speed Limits and Cosmology: Acceleration from D-cceleration
- The primordial density perturbation in the curvaton scenario
- Second-Order Cosmological Perturbations from Inflation
- Ghost Inflation
- The Three--Point Correlation Function of the Cosmic Microwave Background in Inflationary Models
- Flavour Issues in Leptogenesis
- k-Essence, superluminal propagation, causality and emergent geometry
- Primordial non-gaussianities in single field inflation
- Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
- Inflation from Warped Space
- Multi-Throat Brane Inflation
- Enhancing the tensor-to-scalar ratio in simple inflation
- Non-gaussianity in fluctuations from warm inflation
- Non-Gaussian Signatures in the Cosmic Background Radiation from Warm Inflation
- Perturbative and non-perturbative aspects of pure N=1 super Yang-Mills theory from wrapped branes
- Seed perturbations for primordial magnetic fields from MSSM flat directions
- Inflation models after WMAP year three
- The Pursuit of Non-Gaussian Fluctuations in the Cosmic Microwave Background
- Constraints on the spectral index for the inflation models in string landscape
- A Stochastic Measure for Eternal Inflation
- Weak gravity conjecture constraints on inflation
- Testing models of inflation with CMB non-gaussianity
Cited by in corpus (49)
- Primordial Non-Gaussianities from Inflation Models
- Quasi-Single Field Inflation and Non-Gaussianities
- Hunting for Primordial Non-Gaussianity in the Cosmic Microwave Background
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- Inflation with multiple sound speeds: a model of multiple DBI type actions and non-Gaussianities
- Curvaton with Polynomial Potential
- Primordial Non-Gaussianities of General Multiple Field Inflation
- On Classification of Models of Large Local-Type Non-Gaussianity
- 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
- The Curvature Perturbation in the Axion-type Curvaton Model
- Reconstructing a general inflationary action
- Second-order matter perturbations in a LambdaCDM cosmology and non-Gaussianity
- Large Primordial Trispectra in General Single Field Inflation
- The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
- Non-Gaussianity and Secondary Gravitational Waves from Primordial Black Holes Production in -attractor Inflation
- Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
- Non-Gaussianity in single field models without slow-roll
- The Trispectrum in the Multi-brid Inflation
- -vacuum and inflationary bispectrum
- N-vaton
- Multi-Stream Inflation
- Consistency Relations for Non-Gaussianity
- Non-canonical generalizations of slow-roll inflation models
- Non-Gaussianities of Single Field Inflation with Non-minimal Coupling
- Warm DBI inflation with constant sound speed
- Non-Gaussianity, Isocurvature Perturbation, Gravitational Waves and a No-Go Theorem for Isocurvaton
- Spectral Index in Curvaton Scenario
- Resurrecting the Power-law, Intermediate, and Logamediate Inflations in the DBI Scenario with Constant Sound Speed
- Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
- Quadra-Spectrum and Quint-Spectrum from Inflation and Curvaton Models
- Mimetic DBI Inflation in Confrontation with Planck2018 data
- Revisiting non-Gaussianity of multiple-field inflation from the field equation
- Thermal fluctuations in viscous cosmology
- Galileon intermediate inflation
- Non-Gaussian Shape Recognition
- Thermal non-Gaussianity in holographic cosmology
- Reconstructing Single Field Inflationary Actions From CMBR Data
- A weak lensing view on primordial non-Gaussianities
- Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
- 1/R Correction to Gravity in the Early Universe
- The interplay of CMB temperature lensing power reconstruction with primordial non-Gaussianity of local type
- Reconstruction of the isocurvaton scenario
- Principal Components of CMB non-Gaussianity
- K-essence Explains a Lorentz Violation Experiment
- Viable Intermediate Inflation in the Mimetic DBI Model
- Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings
- Revisiting the angular momentum growth of protostructures evolved from non-Gaussian initial conditions