Solutions for f(R) gravity coupled with electromagnetic field
arXiv:1110.5085 · doi:10.1140/epjc/s10052-011-1851-7
Abstract
In the presence of external, linear / nonlinear electromagnetic fields we integrate f(R) \sim R+2α\surd(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.
7 pages no figure, final version for publication in European Physical Journal C
References in corpus (4)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Friedmann Equations of FRW Universe in Scalar-tensor Gravity, f(R) Gravity and First Law of Thermodynamics
- Confinement from spontaneous breaking of scale symmetry
- Static potential from spontaneous breaking of scale symmetry
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