Power-counting during single-field slow-roll inflation

DOI10.1088/1475-7516/2018/02/016OpenAlexW2747267371MaRDI QIDQ5022075

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Publication date: 18 January 2022

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

Full work available at URL: https://arxiv.org/abs/1708.07443

zbMATH Keywords

inflationphysics of the early universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (6)

Keeping an eye on DBI: power-counting for small-c_s cosmology ⋮ Inflation in motion: unitarity constraints in effective field theories with (spontaneously) broken Lorentz symmetry ⋮ Yoga Dark Energy: natural relaxation and other dark implications of a supersymmetric gravity sector ⋮ Quantum corrections to the primordial tensor spectrum: open EFTs \& Markovian decoupling of UV modes ⋮ Minimal decoherence from inflation ⋮ Non-Gaussianity from entanglement during inflation

Cites Work

• The quantum Fokker-Planck equation of stochastic inflation
• EFT beyond the horizon: stochastic inflation and how primordial quantum fluctuations go classical
• Quantum gravity in everyday life: general relativity as an effective field theory
• On Higgs inflation and naturalness
• A new type of isotropic cosmological models without singularity
• Quantum diffusion during inflation and primordial black holes
• Productive interactions: heavy particles and non-Gaussianity
• Stochastic inflation in phase space: is slow roll a stochastic attractor?
• Inflationary universe: A possible solution to the horizon and flatness problems
• Quantum Theory of Gravity. I. The Canonical Theory
• Quantum Theory of Gravity. II. The Manifestly Covariant Theory

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