Inflation after preheating
Creators
- 1. E-mail: linde at hbar.Stanford.EDU (United States)
Description
Preheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with the vacuum energy in the state with restored symmetry. As a result, in some inflationary models one encounters a secondary, nonthermal stage of inflation due to symmetry restoration after preheating. We review the theory of nonthermal phase transitions and make a prediction about the expansion factor during the secondary inflationary stage. We then present the results of lattice simulations which verify these predictions, and discuss possible implications of our results for the theory of formation of topological defects during nonthermal phase transitions. (author)
Additional details
Publishing Information
- Journal Title
- Journal of High Energy Physics (Online)
- Journal Volume
- 08
- Journal Issue
- 2000
- Journal Page Range
- p. vp
- ISSN
- 1029-8479
INIS
- Country of Publication
- Italy
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43112398
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMOLOGY; ENERGY DENSITY; INFLATIONARY UNIVERSE; LATTICE FIELD THEORY; PHASE TRANSFORMATIONS
- Descriptors DEC
- CONSTRUCTIVE FIELD THEORY; COSMOLOGICAL MODELS; FIELD THEORIES; MATHEMATICAL MODELS; QUANTUM FIELD THEORY
Optional Information
- Notes
- Available in electronic form only at the Web site of the Journal of High Energy Physics located at http:/jhep.sissa.it/. E-print number: hep-ph/0004024; This record replaces 31041943