Evolution of the very early universe with polarized vacuum
β Scribed by V. G. Gurzadyan; A. A. Kocharyan; S. G. Matinyan
- Publisher
- Springer
- Year
- 1985
- Tongue
- English
- Weight
- 276 KB
- Volume
- 22
- Category
- Article
- ISSN
- 0571-7256
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Homogeneous isotropic cosmological models driven a t early timcs by a colicrent scalar [ield and the vacuuni polarization arc consitlrretl. Roth effects can lead t o the existence of a finite minimal value of the scale factor and an inflationary stage of expansion. The early as well as the late time
Interaction of scalar fields Time dependent temperature Lorentz invariant temperature inflation field Temperature decrease and increase in the inflationary and reheating period a b s t r a c t We consider a scalar field Ο which acts as a potential function to generate a (thermo)dynamic temperature