Reconstructing f(R) theory according to holographic dark energy
| dc.creator | Wu, Xing | |
| dc.creator | Zhu, Zong-Hong | |
| dc.date | 2007-12-21 | |
| dc.date | 2007-12-23 | |
| dc.date.accessioned | 2026-07-07T11:13:52Z | |
| dc.date.available | 2026-07-07T11:13:52Z | |
| dc.description | In this paper a connection between the holographic dark energy model and the $f(R)$ theory is established. We treat the $f(R)$ theory as an effective description for the holographic dark energy and reconstruct the function $f(R)$ with the parameter $c>1$, $c=1$ and $c<1$, respectively. We show the distinctive behavior of each cases realized in $f(R)$ theory, especially for the future evolution. | |
| dc.description | 6 pages, 4 figures, accepted for publication in Physics Letters B | |
| dc.identifier | https://arxiv.org/abs/0712.3603 | |
| dc.identifier | http://arxiv.org/abs/0712.3603 | |
| dc.identifier | Phys.Lett.B660:293-298,2008 | |
| dc.identifier | doi:10.1016/j.physletb.2007.12.031 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/191872 | |
| dc.subject | Astrophysics | |
| dc.title | Reconstructing f(R) theory according to holographic dark energy | |
| dc.type | text |