Physical Significance of the Difference between the Brans-Dicke Theory and General Relativity
| dc.creator | Miyazaki, A. | |
| dc.date | 2000-12-28 | |
| dc.date.accessioned | 2026-07-07T03:25:33Z | |
| dc.date.available | 2026-07-07T03:25:33Z | |
| dc.description | The asymptotic behavior of the scalar field and its physical meaning are discussed for T=0 and T\neq 0 for the large enough coupling parameter ω. The special character of the Brans-Dicke theory is also discussed for local and cosmological problems in comparison with general relativity and the selection rules are introduced respectivley. The scalar field by locally-distributed matter should exhibit the asymptotic behavior ϕ= <ϕ> +O(1/ω) because of the presence of cosmological matter. The scalar field of a proper cosmological solution should have the asymptotic form ϕ=O(ρ/ω) and should converge to zero in the continuous limit ρ/ω\to 0. | |
| dc.description | 13 pages, LaTeX2e. Submitted to Physical Review D | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0012104 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0012104 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33751 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Physical Significance of the Difference between the Brans-Dicke Theory and General Relativity | |
| dc.type | text |