Chen-Wu type model and the total energy of the universe
| dc.creator | de Campos, M. | |
| dc.date | 2004-10-16 | |
| dc.date.accessioned | 2026-07-07T03:29:04Z | |
| dc.date.available | 2026-07-07T03:29:04Z | |
| dc.description | The inclusion of a $Λ$ term, today, in the relativistic field equations is consequence of the evolution of an observational cosmology. In this work we argue the "ansatz" $Λ= βH^2 +\fracα{R^2}$ is applicable to the total energy density of the universe, discuss some cosmological consequences and compare the growing mode of the density contrast with the corresponding mode of the standard model. | |
| dc.description | 10 pages, 5figures. XXV National Meeting of Particles and Fields Physics | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0410075 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0410075 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35072 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Chen-Wu type model and the total energy of the universe | |
| dc.type | text |