Optimized numerical evolution of perturbations across sharp background trajectory turns in multifield inflation
gr-qc, astro-ph.CO, hep-th
Submitted: 2026-03-28
Updated: 2026-10-07
Comments: 24+1 pages, 10 figures, 3 ancillary animations, comments are welcome
Journal ref: JCAP10(2026)019
DOI: 10.1088/1475-7516/2026/10/019
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Summary of Results from COBE
- Planck 2018 results. X. Constraints on inflation
- The Simons Observatory: Science goals and forecasts
- CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
- CMB-S4: Iterative Internal Delensing and $r$ Constraints
- The Simons Observatory: Combining delensing and foreground cleaning for improved constraints on inflation
- Cosmological Attractors and Asymptotic Freedom of the Inflaton Field
- On hilltop and brane inflation after Planck
- Hybrid cosmological attractors
- Inflationary $\alpha$-Attractor From Type IIB/F Theory
- Geometrical Destabilization of Inflation
- Higgs-Dilaton Cosmology: From the Early to the Late Universe
- Random Potentials and Cosmological Attractors
- Multi-field Inflation in High-Slope Potentials
- Sharp turns in axion monodromy: primordial black holes and gravitational waves
- The Trans-Planckian Problem of Inflationary Cosmology
- Observational Constraints on Constant Roll Inflation
- Two-point correlators revisited: Fast and slow scales in multifield models of inflation
- TASI Lectures on Inflation
- The Effective Field Theory of Inflation Models with Sharp Features
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