Double inflation via non-minimally coupled spectator

DOI10.1088/1475-7516/2022/06/016zbMath1505.83040arXiv2202.04869OpenAlexW4221146538MaRDI QIDQ5099328

Kin-Ya Oda, Mio Kubota, Stanislav Rusak, Tomo Takahashi

Publication date: 31 August 2022

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

Full work available at URL: https://arxiv.org/abs/2202.04869

zbMATH Keywords

inflationcosmological perturbation theoryphysics of the early universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Perturbations in context of PDEs (35B20) Strange attractors, chaotic dynamics of systems with hyperbolic behavior (37D45) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Adiabatic invariants for problems in Hamiltonian and Lagrangian mechanics (70H11)

Related Items (3)

Effective field theory of magnetogenesis identify necessary and sufficient conditions ⋮ Non-minimally assisted chaotic inflation ⋮ Nonminimally assisted inflation: a general analysis

Cites Work

• Frame covariant nonminimal multifield inflation
• Hillclimbing inflation in metric and Palatini formulations
• Quantum Field Theory in Curved Spacetime
• Higgs inflation with loop corrections in the Palatini formulation
• Resurrecting Quadratic Inflation with a non-minimal coupling to gravity
• Natural Inflation with a periodic non-minimal coupling
• Natural inflation with a nonminimal coupling to gravity
• Non-minimally coupled curvaton
• Reheating in models with non-minimal coupling in metric and Palatini formalisms
• Higgs inflation in metric and Palatini formalisms: required suppression of higher dimensional operators
• Rollercoaster cosmology
• Generating primordial features at large scales in two field models of inflation
• Rescuing quartic and natural inflation in the Palatini formalism
• Towards distinguishing variants of non-minimal inflation
• Quantum Fields in Curved Space
• Effects of cosmological moduli fields on cosmic microwave background
• Generating the curvature perturbation without an inflaton

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