Solutions for f(R) gravity coupled with electromagnetic field

In the presence of external, linear/nonlinear electromagnetic fields we integrate f (R) similar to R+ 2 alpha root R + const. gravity equations. In contrast to their Einsteinian cousins the obtained black holes are non-asymptotically flat with a deficit angle. In proper limits we obtain from our general solution the global monopole solution in f (R) gravity. The scale symmetry breaking term adopted as the nonlinear electromagnetic source adjusts the sign of the mass of the resulting black hole to be physical.