Journal
PHYSICAL REVIEW LETTERS
Volume 85, Issue 11, Pages 2236-2239Publisher
AMERICAN PHYSICAL SOC
DOI: 10.1103/PhysRevLett.85.2236
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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).
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