Quantum Standard Clocks in the Primordial Trispectrum
arXiv:1803.04412 · doi:10.1088/1475-7516/2018/05/049
Abstract
We calculate the primordial trispectrum of curvature perturbation in quasi-single field inflation, with general sound speeds for both the inflaton and the massive scalar. Special attention is paid to various soft limits of the trispectrum, where the shape function shows characteristic oscillatory pattern (known as the quantum primordial standard clock signal) as a function of the momentum ratio. Our calculation is greatly simplified by using the "mixed propagator" developed under a diagrammatic representation of the in-in formalism.
arXiv comment23 pages, JCAP accepted version
References in corpus (39)
- Non-Gaussianity from Inflation: Theory and Observations
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Primordial Non-Gaussianities from Inflation Models
- Quasi-Single Field Inflation and Non-Gaussianities
- Signatures of Supersymmetry from the Early Universe
- On Soft Limits of Inflationary Correlation Functions
- Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation
- Effective field theory approach to quasi-single field inflation and effects of heavy fields
- Non-Gaussianity as a Particle Detector
- The Gelaton Scenario: Equilateral non-Gaussianity from multi-field dynamics
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- Effective theories of single field inflation when heavy fields matter
- Quasi-Single Field Inflation with Large Mass
- Schwinger-Keldysh Diagrammatics for Primordial Perturbations
- Inflation, Cosmic Perturbations and Non-Gaussianities
- Strongly Coupled Perturbations in Two-Field Inflationary Models
- Standard Model Background of the Cosmological Collider
- Prospects for Cosmological Collider Physics
- Loop Corrections to Standard Model Fields in Inflation
- Standard Model Mass Spectrum in Inflationary Universe
- Equilateral non-Gaussianity from heavy fields
- Inflation with multiple sound speeds: a model of multiple DBI type actions and non-Gaussianities
- Imprints of Massive Primordial Fields on Large-Scale Structure
- On the full trispectrum in single field DBI-inflation
- Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background
- Galaxy Bispectrum from Massive Spinning Particles
- A Naturally Large Four-Point Function in Single Field Inflation
- Models of the Primordial Standard Clock
- Standard Clock in Primordial Density Perturbations and Cosmic Microwave Background
- Fingerprints of Primordial Universe Paradigms as Features in Density Perturbations
- Imprints of Spinning Particles on Primordial Cosmological Perturbations
- Strongly Coupled Quasi-Single Field Inflation
- Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias
- Searching for Standard Clocks in the Primordial Universe
- High Energy Physics Signatures from Inflation and Conformal Symmetry of de Sitter
- On the Effective Field Theory for Quasi-Single Field Inflation
- Spectroscopy of Masses and Couplings during Inflation
- Feeding your Inflaton: Non-Gaussian Signatures of Interaction Structure
- A Direct Probe of the Evolutionary History of the Primordial Universe
Cited by in corpus (19)
- In Search of Large Signals at the Cosmological Collider
- Neutrino Signatures in Primordial Non-Gaussianities
- No-go Theorem for Scalar-Trispectrum-Induced Gravitational Waves
- Cutting Rule for Cosmological Collider Signals: A Bulk Evolution Perspective
- Phase Information in Cosmological Collider Signals
- Helical Inflation Correlators: Partial Mellin-Barnes and Bootstrap Equations
- Bootstrapping One-Loop Inflation Correlators with the Spectral Decomposition
- Closed-Form Formulae for Inflation Correlators
- Landscape tomography through primordial non-Gaussianity
- Classical Cosmological Collider Physics and Primordial Features
- Continuous Spectrum on Cosmological Collider
- Decoherence out of fire: Purity loss in expanding and contracting universes
- Cosmological Angular Trispectra and Non-Gaussian Covariance
- Analytic Formulae for Inflationary Correlators with Dynamical Mass
- The Massive Flat Space Limit of Cosmological Correlators
- Fingerprints of a Non-Inflationary Universe from Massive Fields
- Schwinger-Keldysh mechanism in extended quasi single field inflation
- Amplifying the Cosmological Collider with Ghost Spectators
- Non-relativistic Cosmological Collider Signals