Simple single-field inflation models with arbitrarily small tensor/scalar ratio
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Publication:6100401
DOI10.1088/1475-7516/2023/03/027zbMath1522.83308arXiv2210.05757OpenAlexW4323660840MaRDI QIDQ6100401
William H. Kinney, Nina K. Stein
Publication date: 12 May 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2210.05757
inflationparticle physics-cosmology connectioncosmological parameters from CMBRinflation and CMBR theory
Unified quantum theories (81V22) Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Quantum optics (81V80)
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Squeezed bispectrum and one-loop corrections in transient constant-roll inflation ⋮ On the constant roll complex scalar field inflationary models
Cites Work
- On the geometry of the string landscape and the swampland
- Unification of constant-roll inflation and dark energy with logarithmic \(R^{{2}}\)-corrected and exponential \(F(R)\) gravity
- On non-slow roll inflationary regimes
- A new type of isotropic cosmological models without singularity
- Constant-roll inflation in F( R ) gravity
- New perspectives on constant-roll inflation
- Systematics of constant roll inflation
- On the constant-roll inflation
- Constant-roll inflation in f(T) teleparallel gravity
- Constant-roll tachyon inflation and observational constraints
- Constant-roll (quasi-)linear inflation
- Revisiting non-Gaussianity from non-attractor inflation models
- A generalized non-Gaussian consistency relation for single field inflation
- Vanishing of local non-Gaussianity in canonical single field inflation
- Stochastic inflation in phase space: is slow roll a stochastic attractor?
- Inflationary universe: A possible solution to the horizon and flatness problems
- Dynamical analysis of attractor behavior in constant roll inflation
- Curvature perturbation at the local extremum of the inflaton potential
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