Small field polynomial inflation: reheating, radiative stability and lower bound

DOI10.1088/1475-7516/2021/09/012zbMath1486.83136arXiv2104.03977OpenAlexW3156165060MaRDI QIDQ5061956

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Publication date: 14 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2104.03977

zbMATH Keywords

inflationphysics of the early universeparticle physics-cosmology connection

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Nuclear physics (81V35) Geometrodynamics and the holographic principle (83E05) Classical and relativistic thermodynamics (80A10) Perturbations in context of PDEs (35B20) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Particle exchange symmetries in quantum theory (general) (81V72)

Uses Software

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Cites Work

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• \texttt{LATTICEEASY}: A program for lattice simulations of scalar fields in an expanding universe
• Radiative plateau inflation
• Inflection-point inflation with axion dark matter in light of trans-Planckian censorship conjecture
• Axion monodromy inflation with warped KK-modes
• A new type of isotropic cosmological models without singularity
• Nonperturbative dynamics of reheating after inflation: A review
• Reheating After Inflation
• Robustness of inflation to inhomogeneous initial conditions
• Expectations for inflationary observables: simple or natural?
• The Primordial Density Perturbation
• Inflationary universe: A possible solution to the horizon and flatness problems
• Flattening the inflaton's potential with quantum corrections

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