Hoyle, F. ; Narlikar, J. V. (1966) A radical departure from the 'steady state' concept in cosmology Proceedings of the Royal Society A: Mathematical, Physical & Engineering Sciences, 290 (1421). pp. 162-176. ISSN 1364-5021
Full text not available from this repository.
Official URL: http://rspa.royalsocietypublishing.org/content/290...
Related URL: http://dx.doi.org/10.1098/rspa.1966.0043
Abstract
The results in this paper are based on an entirely different choice of the undetermined coupling constant f which appears in the theory of creation of matter. Previously f was chosen to make the steady-state expansion rate coincident with the observed expansion rate. Now that we take a much larger value for f, the corresponding steady-state expansion rate is much greater than the observed value. We interpret this difference as showing that we live in a wide, possibly temporary, fluctuation from the steady-state situation. The expansion rate in such a fluctuation follows the Einstein-de Sitter relations. The natural scale set by the new steady-state corresponds to the masses of clusters of galaxies, we obtain 1013M⊙ instead of 1023M⊙ for the 'observable universe'. It is suggested that elliptical galaxies were formed early in the development of a fluctuation. Our discussion of high energy phenomena leads to immediate explanations of the energy spectrum of cosmic rays, of the presence of e+ in cosmic rays and of the rate of energy production associated with radio sources.
Item Type: | Article |
---|---|
Source: | Copyright of this article belongs to The Royal Society. |
ID Code: | 41181 |
Deposited On: | 27 May 2011 05:55 |
Last Modified: | 27 May 2011 05:55 |
Repository Staff Only: item control page