Abstract
We study some features of static and spherically symmetric solutions (SSS) with a horizon in theories of gravitation by means of a near-horizon analysis. A necessary condition for an theory to have this type of solution is obtained. General features of the effective potential are deduced, and it is shown that there exists a limit on the curvature at the horizon, in both cases for any . Finally, we calculate the expression for the energy of the collision of two massive particles in the center of mass frame.
- Received 9 August 2011
DOI:https://doi.org/10.1103/PhysRevD.84.084006
© 2011 American Physical Society