Spectroscopy of Masses and Couplings during Inflation
arXiv:1311.0184 · doi:10.1088/1475-7516/2014/04/031
Abstract
In this work, we extend the idea of Quasi Single Field inflation to the case of multiple isocurvaton fields with masses of order of Hubble, which are coupled kinetically to the inflaton field and have some interactions among themselves. We consider the effects of these massive modes in both the size and the shape of the bispectrum. We show that the shape of the bispectrum in the squeezed limit is dominated by the lightest field and is the same as in Quasi Single Field inflation. This is a generic feature of multiple isocurvaton fields and is independent of the details of the interactions among the massive fields. When the isocurvaton fields have similar masses, we can potentially distinguish two different shapes in the squeezed limit so that the shape of the bispectrum can act as a particle detector. However, in the presence of hierarchy among the massive fields, the dominant effect is due to the lightest field.
References added, minor changes, Published in JCAP
References in corpus (10)
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- Primordial Non-Gaussianities from Inflation Models
- String Cosmology: A Review
- Multiple field inflation
- Curvature Perturbation Spectrum in Two-field Inflation with a Turning Trajectory
- Equilateral non-Gaussianity from heavy fields
- Planck-Suppressed Operators
- Inflation induced by Gravitino Condensation in Supergravity
- Oscillatory features in the curvature power spectrum after a sudden turn of the inflationary trajectory
- Observable predictions of generalised inflationary scenarios
Cited by in corpus (33)
- Scalaron from -gravity as a Heavy Field
- Schwinger-Keldysh Diagrammatics for Primordial Perturbations
- Prospects for Cosmological Collider Physics
- Standard Model Background of the Cosmological Collider
- Standard Model Mass Spectrum in Inflationary Universe
- Neutrino Signatures in Primordial Non-Gaussianities
- The Future of Primordial Features with Large-Scale Structure Surveys
- Cosmological Signatures of Superheavy Dark Matter
- Classical Cosmological Collider Physics and Primordial Features
- Landscape tomography through primordial non-Gaussianity
- Disentangling mass spectra of multiple fields in cosmological collider
- Quantum Primordial Standard Clocks
- On the Effective Field Theory for Quasi-Single Field Inflation
- Constraining chameleon field driven warm inflation with Planck 2018 data
- Quantum Standard Clocks in the Primordial Trispectrum
- Heavy Spinning Particles from Signs of Primordial Non-Gaussianities: Beyond the Positivity Bounds
- Warm Quasi-Single Field Inflation
- Axion Isocurvature Collider
- Constant-roll approach to non-canonical inflation
- Continuous Spectrum on Cosmological Collider
- Effective Field Theory of non-Attractor Inflation
- Combined features in the primordial spectra induced by a sudden turn in two-field DBI inflation
- Analytic Formulae for Inflationary Correlators with Dynamical Mass
- Charged Vector Inflation
- Perturbative unitarity in quasi-single field inflation
- On the equation-of-motion versus in-in approach in cosmological perturbation theory
- Non-Gaussianities in a two-field generalization of Natural Inflation
- Non-Gaussianity from gauge bosons in Cosmological Collider Physics
- Dark Matter from Entropy Perturbations in Curved Field Space
- A Universal Bound on Excitations of Heavy Fields during Inflation
- Schwinger-Keldysh mechanism in extended quasi single field inflation
- Massive Fields as Systematics for Single Field Inflation
- On the importance of heavy fields in pseudo-scalar inflation