A numerical analysis for G(t) in a scalar tensor theory
| dc.creator | Trevisan, Luis Augusto | |
| dc.date | 2003-02-03 | |
| dc.date | 2003-02-04 | |
| dc.date.accessioned | 2026-07-07T03:27:36Z | |
| dc.date.available | 2026-07-07T03:27:36Z | |
| dc.description | We calculated the evolution of the Newton gravitational in a scalar tensor theory, using parameters that holds for the present Universe. We analised the evolution from one billion of years ago. | |
| dc.description | The 4 figures (ps files) were included | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0302002 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0302002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34493 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A numerical analysis for G(t) in a scalar tensor theory | |
| dc.type | text |