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 |