Effect of inflation on anisotropic cosmologies
The effects of anisotropic cosmologies on inflation are studied. By properly formulating the field equations it is possible to show that any model that undergoes sufficient inflation will become isotropic on scales greater than the horizon today. Furthermore, we shall show that it takes a very long time for anisotropies to become visible in the observable part of the Universe. It is interesting to note that the time scale will be independent of the Bianchi Model and of the initial anisotropy. 6 refs.
- Research Organization:
- Fermi National Accelerator Lab., Batavia, IL (USA)
- DOE Contract Number:
- AC02-76CH03000
- OSTI ID:
- 6020214
- Report Number(s):
- FNAL/Pub-86/48-A; ON: DE86009993
- Country of Publication:
- United States
- Language:
- English
Similar Records
Effect of inflation on anisotropic cosmologies
Bianchi models and new inflation
Homogeneous cosmological models and new inflation
Journal Article
·
Fri Aug 15 00:00:00 EDT 1986
· Phys. Rev. D; (United States)
·
OSTI ID:5648667
Bianchi models and new inflation
Technical Report
·
Fri Feb 28 23:00:00 EST 1986
·
OSTI ID:5801979
Homogeneous cosmological models and new inflation
Journal Article
·
Sun Oct 26 23:00:00 EST 1986
· Phys. Rev. Lett.; (United States)
·
OSTI ID:6955423