Abstract
We show that the metric in theories of gravity in Palatini formalism can be solved as the product of a rank-two tensor times a scalar function which is very sensitive to the local energy-momentum densities. This local dependence of the metric generates new gravitationally-induced microscopic interactions, which eventually would lead to self-accelerated test body trajectories. These facts make very unlikely the viability of Palatini models designed to change the late-time cosmic evolution.
- Received 6 December 2006
DOI:https://doi.org/10.1103/PhysRevLett.98.061101
©2007 American Physical Society