Inflation models after WMAP year three
arXiv:astro-ph/0603539 · doi:10.1088/1475-7516/2006/08/013
Abstract
The survey of models in astro-ph/0510441 is updated.For the first time, a large fraction of the models is ruled out at more than .
4 pages
References in corpus (1)
Cited by in corpus (26)
- Inflation and WMAP three year data: Features have a Future!
- New Constraints on Oscillations in the Primordial Spectrum of Inflationary Perturbations
- Inflation, dark matter and dark energy in the string landscape
- On the Issue of the ζSeries Convergence and Loop Corrections in the Generation of Observable Primordial Non-Gaussianity in Slow-Roll Inflation. Part I: the Bispectrum
- Generating Primordial Black Holes Via Hilltop-Type Inflation Models
- Natural Inflation: status after WMAP 3-year data
- Inflation over the hill
- Quantum modes in DBI inflation: exact solutions and constraints from vacuum selection
- General Single Field Inflation with Large Positive Non-Gaussianity
- Curvaton reheating allows TeV Hubble scale in NO inflation
- Constraints on the spectral index for the inflation models in string landscape
- Limits on primordial power spectrum resolution: An inflationary flow analysis
- Non-canonical generalizations of slow-roll inflation models
- WMAP-normalized Inflationary Model Predictions and the Search for Primordial Gravitational Waves with Direct Detection Experiments
- Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model
- -exponential inflation
- Constraints on Quintessence From Using Cosmological Data
- Is Cosmology Compatible with Blue Gravity Waves ?
- Cosmological constraints in the presence of ionizing and resonance radiation at recombination
- Flat Tree-level Inflationary Potentials in Light of CMB and LSS Data
- Brane Inflation and the Overshoot Problem
- Slow-roll reconstruction for running spectral index
- Predictions of Dynamically Emerging Brane Inflation Models
- CMB and LSS constraints on a single-field model of inflation
- Radiation Driven Inflation
- Inverted Hybrid Inflation as a solution to gravitino problems in Gravity Mediation