Holography, dark energy and entropy of large cosmic structures

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6315

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	Arun, K	-
dc.date.accessioned	2013-08-20T10:30:55Z	-
dc.date.available	2013-08-20T10:30:55Z	-
dc.date.issued	2013-11	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 348, No. 1, pp 217-219	en
dc.identifier.issn	1572-946X	-
dc.identifier.uri	http://hdl.handle.net/2248/6315	-
dc.description	Restricted Access	en
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	As is well known, black hole entropy is proportional to the area of the horizon suggesting a holographic principle wherein all degrees of freedom contributing to the entropy reside on the surface. In this note, we point out that large scale dark energy (such as a cosmological constant) constraining cosmic structures can imply a similar situation for the entropy of a hierarchy of such objects.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://dx.doi.org/10.1007/s10509-013-1564-5	en
dc.relation.uri	http://arxiv.org/abs/1303.4363	en
dc.rights	© Springer	en
dc.subject	Black hole entropy	en
dc.subject	Holographic principle	en
dc.subject	Cosmological constant	en
dc.title	Holography, dark energy and entropy of large cosmic structures	en
dc.type	Article	en
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