Tracing out massive fields in cosmology
hep-th, astro-ph.CO, hep-ph
Submitted: 2026-09-24
Updated: 2026-09-24
Terminology
Sources
- Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation
- Quasi-Single Field Inflation and Non-Gaussianities
- Quantum Primordial Standard Clocks
- Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background
- Prospects for Cosmological Collider Physics
- Galaxy Bispectrum from Massive Spinning Particles
- Scale-Dependent Galaxy Bias from Massive Particles with Spin during Inflation
- Galaxy Bias and Primordial Non-Gaussianity
- Constraints on long-lived, higher-spin particles from galaxy bispectrum
- Planck 2018 results. IX. Constraints on primordial non-Gaussianity
- Searching for Cosmological Collider in the Planck CMB Data
- BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action
- Cosmological Collider Physics
- Searching for Cosmological Collider in the Planck CMB Data II: collider templates and Modal analysis
- Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data
- Dissecting the Scalar Cosmological Collider with the Cosmic Microwave Background
- Dissipative effects in the Effective Field Theory of Inflation
- EFT Beyond the Horizon: Stochastic Inflation and How Primordial Quantum Fluctuations Go Classical
- An effective field theory during inflation: reduced density matrix and its quantum master equation
- An effective field theory during inflation II: stochastic dynamics and power spectrum suppression
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