Modular Inflation at Higher Level
arXiv:1902.04625 · doi:10.1088/1475-7516/2019/06/036
Abstract
We introduce the framework of modular inflation with level structure, generalizing the level one theory considered previously to higher levels. We analyze the modular structure of CMB observables in this framework and show that the nontrivial geometry of the target space suffices to ensure the almost holomorphic modularity of the relevant parameters. We further introduce a concrete class of models based on hauptmodul functions that provide generators of the corresponding inflationary potentials at level . The phenomenology of this class of models provides targets for ground-based CMB experiments in the immediate future. In the framework of our models we also discuss the status of the quantum gravity conjectures that have been formulated in the context of the swampland.
37 pages, 4 figures
References in corpus (8)
- On the Geometry of the String Landscape and the Swampland
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
- Primordial Bispectrum from Multifield Inflation with Nonminimal Couplings
- Primordial perturbations from inflation with a hyperbolic field-space
- Hyperinflation generalised: from its attractor mechanism to its tension with the `swampland conjectures'
- Multi-field Inflation with a Random Potential
- Testing Two-Field Inflation
Cited by in corpus (8)
- Hyperbolic field space and swampland conjecture for DBI scalar
- Multi-field Inflation in High-Slope Potentials
- Moduli inflation from modular flavor symmetries
- Hidden symmetries of two-field cosmological models
- Large and small field inflation from hyperbolic sigma models
- The infrared behavior of tame two-field cosmological models
- Escape from the swamp with spectator
- Scaling behavior of observables as a model characteristic in multifield inflation