Spinor field with induced nonlinearity in a Bianchi type-I Universe
| dc.creator | Saha, Bijan | |
| dc.date | 2002-12-27 | |
| dc.date.accessioned | 2026-07-07T03:27:27Z | |
| dc.date.available | 2026-07-07T03:27:27Z | |
| dc.description | Self-consistent solutions to the spinor, scalar and BI gravitational field equations are obtained. The problems of initial singularity and asymptotically isotropization process of the initially anisotropic space-time are studied. It is also shown that the introduction of the Cosmological constant ($Λ$-term) in the Lagrangian generates oscillations of the BI model, which is not the case in absence of $Λ$ term. | |
| dc.description | RevTex, 16 pages, 8 figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0212116 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0212116 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34442 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Spinor field with induced nonlinearity in a Bianchi type-I Universe | |
| dc.type | text |