Quasi-Steady State Cosmology - Revision history

Maintenance script: Imported from text file

2017-01-02T02:51:38Z

Imported from text file

← Older revision		Revision as of 22:51, 1 January 2017
Line 13:		Line 13:
	[[Category:Scientific Paper\|quasi-steady state cosmology]]		[[Category:Scientific Paper\|quasi-steady state cosmology]]

	[[Category:Cosmology]]		[[Category:Cosmology\|quasi-steady state cosmology]]

Maintenance script: Imported from text file

2017-01-01T17:57:44Z

Imported from text file

← Older revision		Revision as of 13:57, 1 January 2017
Line 9:		Line 9:
	==Abstract==		==Abstract==

	in <em>Proceedings of Frontiers of the Universe Conference</em>, 17-23 June 2001. A brief historical account of modern cosmology shows that the standard big bang (BB) model, believed by so many, does not have the strong observational foundations that are frequently claimed for it. The theory of the Quasi-Steady State Cosmology (QSSC) and explosive cosmogony is outlined. Comparisons are made between the two theories in explaining the observed properties of the universe, namely, the expansion, chemical composition, CMB, QSO redshifts and explosive events, galaxy formation, and the m-z and theta-z relations. Only two of the observed properties have ever been predicted from the theories (a) the expansion predicted from Einstein's theory by Friedmann and Lemaitre, and (b) the acceleration predicted by the classical steady state theory and the QSSC.[[Category:Scientific Paper]]		in <em>Proceedings of Frontiers of the Universe Conference</em>, 17-23 June 2001. A brief historical account of modern cosmology shows that the standard big bang (BB) model, believed by so many, does not have the strong observational foundations that are frequently claimed for it. The theory of the Quasi-Steady State Cosmology (QSSC) and explosive cosmogony is outlined. Comparisons are made between the two theories in explaining the observed properties of the universe, namely, the expansion, chemical composition, CMB, QSO redshifts and explosive events, galaxy formation, and the m-z and theta-z relations. Only two of the observed properties have ever been predicted from the theories (a) the expansion predicted from Einstein's theory by Friedmann and Lemaitre, and (b) the acceleration predicted by the classical steady state theory and the QSSC.

			[[Category:Scientific Paper\|quasi-steady state cosmology]]

	[[Category:Cosmology]]		[[Category:Cosmology]]

Maintenance script: Imported from text file

2016-12-30T17:05:55Z

Imported from text file

New page

{{Infobox paper
| title = Quasi-Steady State Cosmology
| author = [[Geoffrey Ronald Burbidge]]
| keywords = [[Steady State Cosmology]]
| published = 2001
| journal = [[ArXiv]]
}}

==Abstract==

in <em>Proceedings of Frontiers of the Universe Conference</em>, 17-23 June 2001. A brief historical account of modern cosmology shows that the standard big bang (BB) model, believed by so many, does not have the strong observational foundations that are frequently claimed for it. The theory of the Quasi-Steady State Cosmology (QSSC) and explosive cosmogony is outlined. Comparisons are made between the two theories in explaining the observed properties of the universe, namely, the expansion, chemical composition, CMB, QSO redshifts and explosive events, galaxy formation, and the m-z and theta-z relations. Only two of the observed properties have ever been predicted from the theories (a) the expansion predicted from Einstein's theory by Friedmann and Lemaitre, and (b) the acceleration predicted by the classical steady state theory and the QSSC.[[Category:Scientific Paper]]

[[Category:Cosmology]]