How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales
Danilo Artigas, Shi Pi, Takahiro Tanaka, Yuko Urakawa
astro-ph.CO, gr-qc, hep-th
Submitted: 2026-08-04
Updated: 2026-08-10
Comments: 20 pages main text, 4 pages appendix, 8 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Primordial Black Holes as Dark Matter
- Primordial Black Holes as Dark Matter: Recent Developments
- Primordial Black Holes as a dark matter candidate
- Primordial Black Holes
- Inflationary perturbations near horizon crossing
- Enhancement of superhorizon scale inflationary curvature perturbations
- Horizon crossing and inflation with large \eta
- Curvature perturbation at the local extremum of the inflaton's potential
- Ultra slow-roll inflation demystified
- The attractive behaviour of ultra-slow-roll inflation
- Primordial Black Hole Formation in Starobinsky's Linear Potential Model
- Inflationary relics from an Ultra-Slow-Roll plateau
- Natura Non Facit Saltum: An Analytical Model of Smooth Slow-Roll to Ultra-Slow-Roll Transition
- Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
- Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach
- Ultra-Slow-Roll Inflation on the Lattice I: Backreaction and Nonlinear Effects
- Ultra-Slow-Roll Inflation on the Lattice II: Nonperturbative Curvature Perturbation
- Constraining Primordial Black Hole Formation from Single-Field Inflation
- Note on the bispectrum and one-loop corrections in single-field inflation with primordial black hole formation
- No-go for the formation of heavy mass Primordial Black Holes in Single Field Inflation
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