The perihelion precession, the deflection of light, and the radar echo delayare classical tests of General Relativity here used to probe brane worldtopologically charged black holes in a f(R) bulk and to constrain the parameterthat arises from the Shiromizu-Maeda-Sasaki procedure applied to a f(R) bulk aswell. The existing Solar system observational data constrain the possiblevalues of the tidal charge parameter and the effective cosmological constantincluding f(R) brane world effects. We show that the observational/experimentaldata for both perihelion precession and radar echo delay make the black holespace of parameters to be more strict than the ones for the Dadhich, Maartens,Papadopoulos and Rezania (DMPR) black hole geometry. Furthermore, thedeflection of light constrains the tidal charge parameter similarly as the DMPRblack holes due to a peculiarity in the equation of motion.
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