LRS Bianchi Type-V Viscous Fluid Universe With a Time Dependent Cosmological Term $Λ$
| dc.creator | Pradhan, Anirudh | |
| dc.creator | Shahi, J. P. | |
| dc.creator | Singh, C. V. | |
| dc.date | 2007-04-06 | |
| dc.date | 2007-08-06 | |
| dc.date.accessioned | 2026-07-07T08:22:00Z | |
| dc.date.available | 2026-07-07T08:22:00Z | |
| dc.description | An LRS Bianchi type-V cosmological models representing a viscous fluid distribution with a time dependent cosmological term $Λ$ is investigated. To get a determinate solution, the viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density. It turns out that the cosmological term $Λ(t)$ is a decreasing function of time, which is consistent with recent observations of type Ia supernovae. Various physical and kinematic features of these models have also been explored. | |
| dc.description | 13 pages, no figure | |
| dc.identifier | https://arxiv.org/abs/0704.0849 | |
| dc.identifier | http://arxiv.org/abs/0704.0849 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/135507 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | LRS Bianchi Type-V Viscous Fluid Universe With a Time Dependent Cosmological Term $Λ$ | |
| dc.type | text |