Charged black holes in a six-dimensional vector-tensor theory
We study a six-dimensional vector-tensor gravitation theory compactified to M_4 x S^2. Here, static spherically-symmetric solutions to the field equations of the theory are investigated. We examine the case that the magnetic charge of the "black hole" is small compared with that located in the "center" of the extra sphere. The Hawking temperature of the black hole is calculated in a simple case.