Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves
Hayato Motohashi, Shi Pi, Yuichiro Tada, Jianing Wang
astro-ph.CO
Submitted: 2026-06-23
Comments: 38 pages, 19 figures
Code: https://github.com/JNWinGH/CR-solver
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Strong Dynamics and Inflation: a review
- Lectures on Inflation
- Initial Conditions for Inflation - A Short Review
- Dynamics of cosmological scalar fields
- Introduction to the number of $e$-folds in slow-roll inflation
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Planck 2018 results. VI. Cosmological parameters
- Planck 2018 results. V. CMB power spectra and likelihoods
- Primordial Black Holes from Inflation and Quantum Diffusion
- Smooth vs instant inflationary transitions: steepest growth re-examined and primordial black holes
- Primordial Black Hole Formation in Starobinsky's Linear Potential Model
- Saddle point inflation from higher order corrections to Higgs/Starobinsky inflation
- Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
- Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
- Revisiting small-scale fluctuations in $\alpha$-attractor models of inflation
- One Small Step for an Inflaton, One Giant Leap for Inflation: a novel non-Gaussian tail and primordial black holes
- Logarithmic Duality of the Curvature Perturbation
- Primordial Black Hole Formation from the Upward Step Model: Avoiding Overproduction
- Eternal inflation near inflection points: a challenge to primordial black hole models
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