The Hypothesis of Cores Retarded during Expansion and the Hot Cosmological Model
Abstract
The existence of bodies with dimensions less than Rg= 2GM/c^2 at the early stages of expansion of the cosmological model leads to a strong accretion of radiation by these bodies. If further calculations will confrim that accretion is catastrophically high, the hypothesis on cores delayed in expansion [3,4] will be in contradiction with observational data.
- Publication:
-
Astronomicheskii Zhurnal
- Pub Date:
- 1966
- Bibcode:
- 1966AZh....43..758Z