Holographic dark energy and late cosmic acceleration
| dc.creator | Pavon, Diego | |
| dc.date | 2006-10-02 | |
| dc.date.accessioned | 2026-07-07T11:04:32Z | |
| dc.date.available | 2026-07-07T11:04:32Z | |
| dc.description | It has been persuasively argued that the number of the effective degrees of freedom of a macroscopic system is proportional to its area rather than to its volume. This entails interesting consequences for cosmology. Here we present a model based on this "holographic principle" that accounts for the present stage of accelerated expansion of the Universe and significantly alleviates the coincidence problem also for non-spatially flat cosmologies. Likewise, we comment on a recently proposed late transition to a fresh decelerated phase. | |
| dc.description | 6 pages, no figures, contribution to the Proceedings of IRGAC-06 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0610008 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0610008 | |
| dc.identifier | J.Phys.A40:6865-6870,2007 | |
| dc.identifier | doi:10.1088/1751-8113/40/25/S31 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/188921 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Holographic dark energy and late cosmic acceleration | |
| dc.type | text |