Uncertainty principle limits on the cosmological constant

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2008-09-24T14:50:33Z	-
dc.date.available	2008-09-24T14:50:33Z	-
dc.date.issued	1986-08	-
dc.identifier.citation	International Journal of Theoretical Physics, Vol. 25, No. 8, pp. 825 - 827	en
dc.identifier.issn	0020-7748	-
dc.identifier.uri	http://hdl.handle.net/2248/3887	-
dc.description	Restricted Access	-
dc.description.abstract	The identification of the cosmological constant term with the energy density of the vacuum enables lower and upper limits to be placed on its value. The upper limit arises from the constraint that the total zero-point energy, which also gravitates, should not dominate cosmological dynamics, while the lower limit can result from the operational requirement that the vacuum-energy shifts over atomic or nuclear scales be at least measurable over Hubble time scales.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00669919	en
dc.subject	Cosmological Constant	en
dc.title	Uncertainty principle limits on the cosmological constant	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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