Journal
EUROPEAN PHYSICAL JOURNAL C
Volume 72, Issue 1, Pages -Publisher
SPRINGER
DOI: 10.1140/epjc/s10052-011-1851-7
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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.
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