Non-standard hierarchies of the runnings of the spectral index in inflation
arXiv:1702.00206 · doi:10.3390/universe3010017
Abstract
Recent analyses of cosmic microwave background surveys have revealed hints that there may be a non-trivial running of the running of the spectral index. If future experiments were to confirm these hints, it would prove a powerful discriminator of inflationary models, ruling out simple single field models. We discuss how isocurvature perturbations in multi-field models can be invoked to generate large runnings in a non-standard hierarchy, and find that a minimal model capable of practically realising this would be a two-field model with a non-canonical kinetic structure. We also consider alternative scenarios such as variable speed of light models and canonical quantum gravity effects and their implications for runnings of the spectral index.
10 pages, conference proceedings for VARCOSMOFUN'16, submitted to special issue "Varying Constants and Fundamental Cosmology" in Universe
References in corpus (8)
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- Curvature and isocurvature perturbations in two-field inflation
- Energy Transfer in Multi Field Inflation and Cosmological Perturbations
- Quantum-gravitational effects on gauge-invariant scalar and tensor perturbations during inflation: The slow-roll approximation
- Power Spectra beyond the Slow Roll Approximation in Theories with Non-Canonical Kinetic Terms
- Quantum Cosmology and the Evolution of Inflationary Spectra
- Effect of transitions in the Planck mass during inflation on primordial power spectra
- Ambiguity in running spectral index with an extra light field during inflation