Equilateral non-Gaussianity from multifield dynamics
Creators
- 1. Perimeter Institute for Theoretical Physics, 31 Caroline St. N, Waterloo, Ontario N2L 2Y5 (Canada)
Description
The distinctive features of single field inflationary models with nonminimal kinetic terms, like Dirac-Born-Infeld and k inflation, can be captured by more familiar multiple-field inflationary systems of the type that typically arise in low-energy supergravity models. At least one heavy field, which we call the gelaton, has an effective potential which depends on the kinetic energy of the inflaton. Integrating out the gelaton gives rise to an effectively single field system for which the speed of sound for the adiabatic fluctuations is reduced, generating potentially observable equilateral non-Gaussianity, while causing negligible isocurvature fluctuations. This mechanism is only active if there is a relatively tight coupling between the gelaton and the inflaton. Requiring that the inflaton-gelaton system remains weakly coupled puts an upper limit on the gelaton mass. This approach gives a potentially UV-completable framework for describing large classes of k-inflationary behavior.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.81.043502;
- arXiv
- arXiv:0910.1853v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 81
- Journal Issue
- 4
- Journal Page Range
- p. 043502-043502.5
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42002417
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BORN-INFELD THEORY; COUPLING; FLUCTUATIONS; INFLATIONARY UNIVERSE; KINETIC ENERGY; MASS; POTENTIALS; SOUND WAVES; SUPERGRAVITY; VELOCITY
- Descriptors DEC
- COSMOLOGICAL MODELS; ENERGY; FIELD THEORIES; MATHEMATICAL MODELS; UNIFIED-FIELD THEORIES; VARIATIONS
Optional Information
- Notes
- (c) 2010 The American Physical Society