The power-law expansion universe and the late-time behavior
| dc.creator | Wei, Yi-Huan | |
| dc.date | 2004-08-12 | |
| dc.date | 2004-11-17 | |
| dc.date.accessioned | 2026-07-07T02:14:16Z | |
| dc.date.available | 2026-07-07T02:14:16Z | |
| dc.description | Using the SNe Ia data we determine the three parameters in the power-law expanding universe model with time-dependent power \cite{W}. Inputting $H_0$ and $t_0$, then we find the $\dot{a}-t$ evolution curve with $m=5.0$ and $q_0=-0.90$ can fit very well to that from SNe observation data. The model predicts the transition redshift $z\simeq0.38$. The dark energy deduced from this model have phantom property but the universe doesn't encounter the Big Rip singularity. Assuming that this model with the three parameters is valid for the future universe, then we predict that the total energy density of the universe is decreasing and will soon reach its minimum. | |
| dc.description | 10 pages, 5 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0408230 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0408230 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8051 | |
| dc.subject | Astrophysics | |
| dc.title | The power-law expansion universe and the late-time behavior | |
| dc.type | text |