Is Cosmology Compatible with Blue Gravity Waves ?
arXiv:0802.1442 · doi:10.1103/PhysRevD.77.101301
Abstract
A primordial gravitational wave background with positive(blue) spectral index is expected in several non-standard inflationary cosmologies where the stress-energy tensor violates the null energy condition. Here we show that a sizable amount of blue gravitational waves is compatible with current cosmological and astrophysical data. So far most of the works on parameter estimation from cosmic microwave background data have assumed a negative or negligible spectral index. The present limits on cosmological parameters, especially on the scalar spectral index, widen up considerably when one allows also for blue tilts of the tensor spectrum. Since the amplitude of the CMB B-mode polarization is larger in these models, future data from Planck are likely to provide crucial measurements.
5 Pages, 5 Figures
References in corpus (31)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- An All-Sky Analysis of Polarization in the Microwave Background
- Statistics of Cosmic Microwave Background Polarization
- Signature of Gravity Waves in Polarization of the Microwave Background
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- A Probe of Primordial Gravity Waves and Vorticity
- Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
- New Ekpyrotic Cosmology
- Producing a Scale-Invariant Spectrum of Perturbations in a Hagedorn Phase of String Cosmology
- Detecting the stochastic gravitational wave background using pulsar timing
- A smooth bouncing cosmology with scale invariant spectrum
- Inflation model constraints from the Wilkinson Microwave Anisotropy Probe three-year data
- Tensor Modes from a Primordial Hagedorn Phase of String Cosmology
- Searching for a Stochastic Background of Gravitational Waves with LIGO
- A Bayesian model selection analysis of WMAP3
- Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
- Implications of a Running Spectral Index for Slow Roll Inflation
- Inflation with violation of the null energy condition
- On the Initial Conditions in New Ekpyrotic Cosmology
- Evolution of gravitational waves through the cosmological QCD transition
- Inflation models after WMAP year three
- Occam's razor meets WMAP
- On the new string theory inspired mechanism of generation of cosmological perturbations
- Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
- Model selection forecasts for the spectral index from the Planck satellite
- WMAP-normalized Inflationary Model Predictions and the Search for Primordial Gravitational Waves with Direct Detection Experiments
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- G-inflation: inflation driven by the Galileon field
- Blue-tilted Tensor Spectrum and Thermal History of the Universe
- Updated Constraints and Forecasts on Primordial Tensor Modes
- Slow-roll Inflation with the Gauss-Bonnet and Chern-Simons Corrections
- Blue Gravity Waves from BICEP2 ?
- A large scale coherent magnetic field: interactions with free streaming particles and limits from the CMB
- Using pulsar timing arrays and the quantum normalization condition to constrain relic gravitational waves
- Swampland Criteria and Constraints on Inflation in a Gravity Theory
- Inflation with exotic kinetic terms in Einstein-Chern-Simons gravity
- Back-Reaction of Gravitational Waves Revisited
- On the prior dependence of constraints on the tensor-to-scalar ratio
- Imprints of relic gravitational waves on pulsar timing