Blue perturbation spectra from inflation
arXiv:astro-ph/9309054 · doi:10.1103/PhysRevD.50.4835
Abstract
We investigate inflationary models leading to density perturbations with a spectral index (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such as those measured by COBE, and that required to give bulk motions and structures on the Mpc scale.
12 pages, plain TEX
References in corpus (10)
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- Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE
- COBE, Gravitational Waves, Inflation and Extended Inflation
- Cosmic Microwave Background Probes Models of Inflation
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Cited by in corpus (27)
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- False Vacuum Inflation with Einstein Gravity
- Reconstructing the Inflaton Potential --- an Overview
- Density Perturbations and Black Hole Formation in Hybrid Inflation
- Black Hole Relics and Inflation: Limits on Blue Perturbation Spectra
- Dilaton Production in String Cosmology
- The Cosmic Microwave Background and Particle Physics
- Constraints from Inflation on Scalar-Tensor Gravity Theories
- More varieties of hybrid inflation
- Constraints on flat cosmologies with tracking Quintessence from Cosmic Microwave Background observations
- Running of the Scalar Spectral Index from Inflationary Models
- Blue Perturbation Spectra from Hybrid Inflation with Canonical Supergravity
- Mirror matter and primordial black holes
- An Inflationary Model with an Exact Perturbation Spectrum
- The spectrum of curvature perturbations from hybrid inflation
- Hybrid Inflation with Quasi-canonical Supergravity
- Gravitational Waves and Primordial Black Holes from Supersymmetric Hybrid Inflation
- Large-scale Perturbations from the Waterfall Field in Hybrid Inflation
- False Vacuum Inflation with a Quartic Potential
- Conditions for Successful Extended Inflation
- Pre-big bang model has Planck problem
- Searching for blue in the dark
- Blue spectra and induced formation of primordial black holes
- Pitfalls of a power-law parameterization of the primordial power spectrum for Primordial Black Hole formation
- Tensor to scalar ratio of perturbation amplitudes and inflaton dynamics
- The roughness of the last scattering surface
- Interpreting Large Scale Structure Observations