Post-Inflationary Dynamics
arXiv:hep-ph/0303175 · doi:10.1088/1475-7516/2004/05/006
Abstract
We argue that -driven inflation must overshoot into an era of deflation. The deflationary period ends quickly with the creation of a hot dense thermal barrier to the forward propagation of quantum correlations from the period of inflationary particle production. Subsequent evolution is controlled by the balance between the persistence of this barrier and the growth in the 4-volume from which such correlations can be seen. This balance can lead to power law expansion.
arXiv comment44 pages, 11 figures
References in corpus (14)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Equilibrium State of a Massless Self-Interacting Scalar Field in the De Sitter Background
- On the Generation of a Scale-Invariant Spectrum of Adiabatic Fluctuations in Cosmological Models with a Contracting Phase
- Super-Acceleration from Massless, Minimally Coupled
- Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
- The Quantum Gravitational Back-Reaction On Inflation
- Quantum Gravity Slows Inflation
- Causality and Cosmic Inflation
- Supernova pencil beam survey
- Perturbative Quantum Gravity And Newton's Law On A Flat Robertson-Walker Background
- Back-Reaction Is For Real
- Matter Contributions to the Expansion Rate of the Universe
- The Quantum Gravitationally Induced Stress Tensor