Observational constraints on the inflaton potential combined with flow-equations in inflaton space
arXiv:hep-ph/0109252 · doi:10.1046/j.1365-8711.2002.05855.x
Abstract
Direct observations provide constraints on the first two derivatives of the inflaton potential in slow roll models. We discuss how present day observations, combined with the flow equations in slow roll parameter space, provide a non-trivial constraint on the third derivative of the inflaton potential. We find a lower bound on the third derivative of the inflaton potential V'''/V > -0.2. We also show that unless the third derivative of the inflaton potential is unreasonably large, then one predicts the tensor to scalar ratio, r, to be bounded from below r > 3 * 10^{-6}.
4 pages, 2 figures. Important sign mistake corrected. Conclusions, abstract and discussion changed
References in corpus (22)
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- Reconstructing the Inflaton Potential --- an Overview
- The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
- A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
- DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum
- The PSCz Catalogue
- Determination of Inflationary Observables by Cosmic Microwave Background Anisotropy Experiments
- COBE, Gravitational Waves, Inflation and Extended Inflation
- A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
- CBR Anisotropy and the Running of the Scalar Spectral Index
- Cosmic microwave background measurements can discriminate among inflation models
- Is cosmology consistent?
- Kinematic Constraints to the Key Inflationary Observables
- Flattening the Inflaton's Potential with Quantum Corrections
- Four-year COBE normalization of inflationary cosmologies
- Flattening the Inflaton's Potential with Quantum Corrections II
- Running-mass models of inflation, and their observational constraints
- Dependence of Inflationary Reconstruction upon Cosmological Parameters
- Scale Dependent Spectral Index in Slow Roll Inflation
- Constraints on inflation from CMB and Lyman-alpha forest
- Probing the power spectrum bend with recent CMB data
- A Signature of Inflation from Dynamical Supersymmetry Breaking
Cited by in corpus (22)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
- Bayesian Analysis of Inflation II: Model Selection and Constraints on Reheating
- A Horizon Ratio Bound for Inflationary Fluctuations
- Bayesian Analysis of Inflation: Parameter Estimation for Single Field Models
- On the inflationary flow equations
- Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
- Implications of the Curvaton on Inflationary Cosmology
- The Knotted Sky II: Does BICEP2 require a nontrivial primordial power spectrum?
- Inflationary potentials yielding constant scalar perturbation spectral indices
- New constraints on the observable inflaton potential from WMAP and SDSS
- Microwave background constraints on inflationary parameters
- Running of the Scalar Spectral Index and Observational Signatures of Inflation
- Stochastic approaches to inflation model building
- Reconstructing large running-index inflaton potentials
- A dark energy view of inflation
- Observational constraint on the fourth derivative of the inflaton potential
- Inflation without inflatons
- Braneworld flow equations
- An updated dark energy view of inflation
- GUT-scale inflation with sizeable tensor modes
- A Brachistochrone Approach to Reconstruct the Inflaton Potential
- Next-generation test of cosmic inflation