Future Universe With w < -1 Without Big Smash
| dc.creator | Srivastava, S. K. | |
| dc.date | 2004-07-02 | |
| dc.date | 2005-05-30 | |
| dc.date.accessioned | 2026-07-07T02:13:42Z | |
| dc.date.available | 2026-07-07T02:13:42Z | |
| dc.description | It is demonstrated that if cosmic dark energy behaves like a fluid with equation of state $p = {\rm w} ρ(p$ and $ρ$ being pressure and energy density respectively) as well as generalized Chaplygin gas simultaneously, Big Rip or Big smash problem does not arise even for equation of state parameter ${\rm w} < -1$.Unlike other phantom models, here, scale factor for the future universe is found regular for all time. | |
| dc.description | 11 pages. To appear in Phys. Lett. B | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0407048 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0407048 | |
| dc.identifier | Phys.Lett. B619 (2005) 1-4 | |
| dc.identifier | doi:10.1016/j.physletb.2005.05.056 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7905 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Future Universe With w < -1 Without Big Smash | |
| dc.type | text |