Thermodynamical picture of the interacting holographic dark energy model
| dc.creator | Setare, M R | |
| dc.date | 2009-02-24 | |
| dc.date.accessioned | 2026-07-07T12:46:11Z | |
| dc.date.available | 2026-07-07T12:46:11Z | |
| dc.description | In the present paper, we provide a thermodynamical interpretation for the holographic dark energy model in a non-flat universe. For this case, the characteristic length is no more the radius of the event horizon ($R_E$) but the event horizon radius as measured from the sphere of the horizon ($L$). Furthermore, when interaction between the dark components of the holographic dark energy model in the non-flat universe is present its thermodynamical interpretation changes by a stable thermal fluctuation. A relation between the interaction term of the dark components and this thermal fluctuation is obtained. | |
| dc.description | 10 pages, contribution to the anniversary volume "The Problems of Modern Cosmology", on the occasion of the 50th birthday of Prof. S. D. Odintsov. Editor: Prof. P. M. Lavrov, Tomsk State Pedagogical University | |
| dc.identifier | https://arxiv.org/abs/0902.4088 | |
| dc.identifier | http://arxiv.org/abs/0902.4088 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/221297 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Thermodynamical picture of the interacting holographic dark energy model | |
| dc.type | text |