1.
Phys Rev Lett
; 85(11): 2236-9, 2000 Sep 11.
Artigo
em Inglês
| MEDLINE
| ID: mdl-10977980
RESUMO
The present acceleration of the Universe strongly indicated by recent observational data can be modeled in the scope of a scalar-tensor theory of gravity. We show that it is possible to determine the structure of this theory along with the present density of dustlike matter from two observable cosmological functions: the luminosity distance and the linear density perturbation in the dustlike matter component as functions of redshift. Explicit results are presented in the first order in the small inverse Brans-Dicke parameter omega(-1).
2.
3.
4.
Phys Rev D Part Fields
; 50(10): 6123-6129, 1994 Nov 15.
Artigo
em Inglês
| MEDLINE
| ID: mdl-10017583
5.
Phys Rev D Part Fields
; 50(10): 6357-6368, 1994 Nov 15.
Artigo
em Inglês
| MEDLINE
| ID: mdl-10017604
6.
Phys Rev D Part Fields
; 50(8): 4827-4834, 1994 Oct 15.
Artigo
em Inglês
| MEDLINE
| ID: mdl-10018133
7.
Phys Rev D Part Fields
; 43(8): 2510-2520, 1991 Apr 15.
Artigo
em Inglês
| MEDLINE
| ID: mdl-10013639