The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models

dc.contributor.author	Sinha, K. P
dc.contributor.author	Sivaram, C
dc.contributor.author	Sudarshan, E. C. G
dc.date.accessioned	2008-10-27T15:16:55Z
dc.date.available	2008-10-27T15:16:55Z
dc.date.issued	1976
dc.identifier.citation	Foundations of Physics, Vol. 6, pp. 717 - 726	en
dc.identifier.issn	0015-9018
dc.identifier.uri	http://hdl.handle.net/2248/3985
dc.description	Restricted Access
dc.description.abstract	Some cosmological consequences of the superfluid vacuum state developed previously by the authors are discussed, particularly with regard to the initial stages of the universe. The transition temperature of the hadronic superfluid (superfluid during the hadron era) is estimated to be 10 /sup 13 K, which is the same as the Hagedorn temperature, giving a physical basis of the thermodynamic bootstrap model.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/jn638w210x444101/	en
dc.subject	cosmology	en
dc.subject	The Universe	en
dc.subject	Hadronic Superfluid	en
dc.subject	Hagedorn Temperature	en
dc.subject	Thermodynamic Bootstrap Model	en
dc.title	The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models	en
dc.type	Article	en