Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-08-04
Phys.Rev.D71:023525,2005
Astronomy and Astrophysics
Astrophysics
20 pages, 4 figures, uses RevTeX
Scientific paper
10.1103/PhysRevD.71.023525
Dark energy candidates for which the equation-of-state parameter w is less than -1 violate the dominant energy condition, and are typically unstable. In scalar-tensor theories of gravity, however, the expansion of the universe can mimic the behavior of general relativity with w<-1 dark energy, without violating any energy conditions. We examine whether this possibility is phenomenologically viable by studying Brans-Dicke models and characterizing both the naturalness of the models themselves, and additional observational constraints from limits on the time-dependence of Newton's constant. We find that only highly contrived models would lead observers to measure w<-1.
Carroll Sean M.
de Felice Antonio
Trodden Mark
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