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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3985

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

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