Dark Entropy: Holographic Cosmic Acceleration
| dc.creator | Linder, Eric V. | |
| dc.date | 2004-10-01 | |
| dc.date.accessioned | 2026-07-07T04:17:34Z | |
| dc.date.available | 2026-07-07T04:17:34Z | |
| dc.description | In cosmic holography, the fundamental quantity is the degrees of freedom on a horizon surface rather than the material contents within the volume. That is, the horizon area and hence cosmological expansion rate H is related to the entropy. Using this as a guide, we examine the consequences of an effective dark {\it entropy} on the past and future dynamics of the universe. The results, including nonmonotonic expansion behavior, are interesting apart from the theoretical motivation. | |
| dc.description | 7 pages, 7 figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/0410017 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0410017 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/52805 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.title | Dark Entropy: Holographic Cosmic Acceleration | |
| dc.type | text |