Inflation in Multi-field Modified DBM Potentials
arXiv:1807.07654 · doi:10.1088/1475-7516/2018/09/042
Abstract
We study multi-field inflation in random potentials generated via a non-equilibrium random matrix theory process. We make a novel modification of the process to include correlations between the elements of the Hessian and the height of the potential, similar to a Random Gaussian Field (RGF). We present the results of over 50,000 inflationary simulations involving 5-100 fields. For the first time, we present results of fields using the full `transport method', without slow-roll approximation. We conclude that Planck compatibility is a common prediction of such models, however significant isocurvature power at the end of inflation is possible.
arXiv comment34 pages, 21 figures. Published version
References in corpus (45)
- Global Optimization by Basin-Hopping and the Lowest Energy Structures of Lennard-Jones Clusters Containing up to 110 Atoms
- A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
- A new approach to the evolution of cosmological perturbations on large scales
- Cosmological perturbations
- Quasi-Single Field Inflation and Non-Gaussianities
- On the Cosmological Implications of the String Swampland
- Super-Horizon Scale Dynamics of Multi-Scalar Inflation
- De Sitter Space and the Swampland
- Features of heavy physics in the CMB power spectrum
- Scalar perturbations during multiple-field slow-roll inflation
- Enhancement of superhorizon scale inflationary curvature perturbations
- Multifield Inflation after Planck: The Case for Nonminimal Couplings
- Curvature and isocurvature perturbations in two-field inflation
- The statistics of critical points of Gaussian fields on large-dimensional spaces
- Strongly Coupled Perturbations in Two-Field Inflationary Models
- Correlated perturbations from inflation and the cosmic microwave background
- Non-linear perturbations in multiple-field inflation
- Primordial Non-Gaussianity in Multi-Scalar Slow-Roll Inflation
- Multifield Inflation after Planck: Isocurvature Modes from Nonminimal Couplings
- Must Cosmological Perturbations Remain Non-Adiabatic After Multi-Field Inflation?
- Non-linear inflationary perturbations
- Universality of multi-field -attractors
- Multifield Cosmological Perturbations at Third Order and the Ekpyrotic Trispectrum
- Moment transport equations for non-Gaussianity
- The exact numerical treatment of inflationary models
- Density perturbations arising from multiple field slow-roll inflation
- Moment transport equations for the primordial curvature perturbation
- Charting an Inflationary Landscape with Random Matrix Theory
- The Importance of Slow-roll Corrections During Multi-field Inflation
- On Gaussian Random Supergravity
- Simple emergent power spectra from complex inflationary physics
- Numerical calculation of second order perturbations
- Efficient diagrammatic computation method for higher order correlation functions of local type primordial curvature perturbations
- Manyfield Inflation in Random Potentials
- Inflation in random Gaussian landscapes
- Seven Lessons from Manyfield Inflation in Random Potentials
- Initial conditions for slow-roll inflation in a random Gaussian landscape
- Hessian eigenvalue distribution in a random Gaussian landscape
- Effect of reheating on predictions following multiple-field inflation
- Counting Vacua in Random Landscapes
- Local random potentials of high differentiability to model the Landscape
- Inflation in multi-field random Gaussian landscapes
- Random Functions via Dyson Brownian Motion: Progress and Problems
- Inflation on a Slippery Slope
- Testing Two-Field Inflation
Cited by in corpus (13)
- The asymptotic dS Swampland Conjecture - a simplified derivation and a potential loophole
- Primordial non-Gaussianity from ultra slow-roll Galileon inflation
- Scaling limits of dS vacua and the swampland
- Draining the Swampland
- The swampland conjecture and the Higgs expectation value
- Multi-field Inflation in High-Slope Potentials
- Towards a complete mass spectrum of type-IIB flux vacua at large complex structure
- Modular Inflation at Higher Level
- Learning to Inflate
- (Slow-)Twisting inflationary attractors
- Many-field Inflation: Universality or Prior Dependence?
- Scaling behavior of observables as a model characteristic in multifield inflation
- Investigation of a kind of neutrino mass matrix