Published 1987 | Version v1
Book

Inflationary universe models and the formation of structure

Description

The main features of inflationary universe models are briefly reviewed. Inflation provides a mechanism which produces energy density fluctuations on cosmological scales. In the original models, it was not possible to obtain the correct magnitude of these fluctuations without fine tuning the particle physics models. Two mechanisms, chaotic inflation, and a dynamical relaxation process are discussed by which inflation may be realized in models which give the right magnitude of fluctuations. 22 references

Additional details

Publishing Information

Publisher
Springer-Verlag.
Imprint Place
New York, NY (USA)
Imprint Title
Nearly normal galaxies: from the Planck time to the present; Proceedings of the Eighth Santa Cruz Summer Workshop in Astronomy and Astrophysics, Santa Cruz, CA, July 21-Aug. 1, 1986
Journal Page Range
p. 355-366.

Conference

Title
nearly normal galaxies: from the Planck time to the present.
Acronym
8. Santa Cruz summer workshop in astronomy and astrophysics
Dates
21 Jul - 1 Aug 1986.
Place
Santa Cruz, CA (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
19057128
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMOLOGY; GRAND UNIFIED THEORY; INFLATIONARY UNIVERSE; RELICT RADIATION; SPACE-TIME
Descriptors DEC
COSMOLOGICAL MODELS; ELECTROMAGNETIC RADIATION; FIELD THEORIES; MATHEMATICAL MODELS; MICROWAVE RADIATION; PARTICLE MODELS; QUANTUM FIELD THEORY; RADIATIONS; UNIFIED GAUGE MODELS