Published 1987
| Version v1
Book
Inflationary universe models and the formation of structure
Creators
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