Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys
Si-Xiang Yang, Oliver H. E. Philcox
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-07-16
Comments: 24 pages, 7 figures. Comments welcome!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- How Gaussian can our Universe be?
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Non-Gaussianity from Inflation: Theory and Observations
- Generating the curvature perturbation without an inflaton
- Adiabatic CMB perturbations in pre-big bang string cosmology
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- The Effective Field Theory of Inflation
- Running Non-Gaussianities in DBI Inflation
- Enhanced Non-Gaussianity from Excited Initial States
- Signatures of Initial State Modifications on Bispectrum Statistics
- Bispectrum signatures of a modified vacuum in single field inflation with a small speed of sound
- Non-Gaussianity from Excited Initial Inflationary States
- Optimal CMB estimators for bispectra from excited states
- Extracting New Physics from the CMB
- Decoupling in an expanding universe: boundary RG-flow affects initial conditions for inflation
- Folded Resonant Non-Gaussianity in General Single Field Inflation
- Looking for non-Gaussianity in all the right places: A new basis for non-separable bispectra
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